The galaxy presents as a relatively smooth, elliptical or lenticular structure. Its morphology is predominantly characterized by a lack of distinct spiral arms or prominent features. There may be a slight asymmetry to the galaxy's shape, with it being slightly elongated. The color gradient suggests an older stellar population, concentrated in the central bulge. Little to no blue color is visible. A faint, diffuse halo surrounds the brighter core, indicating a smooth transition of stellar density outwards. There is no strong evidence of an ongoing major merger, though a slight irregular shape may suggest minor past disturbances.
