The galaxy presents an elongated morphology, appearing cigar-shaped. It exhibits a smooth profile with a dominant central bulge that transitions into a slightly extended disk. The color distribution suggests an older stellar population, with a reddish hue concentrated in the central regions and a gradual shift to slightly bluer tones in the outer portions of the disk. There is an indication of a possible minor interaction or tidal disturbance in the form of a faint, diffuse structure. The general form suggests that the galaxy may be undergoing, or has recently undergone, some type of interaction. The light distribution suggests that this galaxy may be in an intermediate stage of evolution.
