The galaxy presents a generally smooth appearance, lacking any immediately discernible spiral arms or significant substructure. Its light distribution appears concentrated toward the center, forming a bright, somewhat elliptical core. The light then gradually fades towards the outer edges of the galaxy, suggesting a relatively homogenous stellar population and dust distribution. The overall color is subtly reddish, which may indicate an older stellar population and subdued star formation activity, possibly with a small amount of dust extinction. There are some subtle irregularities in the outer regions, suggesting some kind of disturbances or interactions. The galaxy's shape is moderately elongated, not perfectly spherical, and not so much that it appears to be cigar-shaped.
