The galaxy presents as a generally smooth, elliptical structure with no apparent spiral arms or a well-defined disk. It appears highly spheroidal in shape, with a significant fraction of its light concentrated in the central region.

The color profile suggests an older stellar population, with a prominent yellowish hue in the core, possibly indicating a higher density of evolved stars. Fainter bluish tints are visible at the edges of the galaxy.

There is no evidence of ongoing major merging activity.
