The galaxy presents a complex morphology, appearing to consist of two distinct components. The primary component is a relatively bright, elongated structure, likely a disk galaxy viewed at a slight angle. The color profile suggests an older stellar population, exhibiting a yellowish hue, with the central bulge appearing more concentrated and intensely colored. The disk shows some irregularity and a slight asymmetry in its outer regions, possibly indicating interactions or tidal disturbances.

A secondary component is located nearby. It is smaller, more spheroidal in shape, and has a smoother texture. Its color is also yellowish, suggesting a similar older stellar population. The proximity of the secondary component and the observed disturbances in the primary galaxy's disk suggest a possible gravitational interaction or ongoing merger event. There appears to be a stream of material connecting the two galaxies in an arc. The tidal features suggest this is an intermediate stage of a merger.

The overall appearance indicates a galaxy that is likely in a relatively quiescent state of star formation.
