The galaxy presents as a relatively smooth, centrally concentrated object. Its overall form appears nearly circular, exhibiting a high degree of roundness in its visual morphology. A dominant central bulge is apparent, marked by a bright, concentrated luminosity. A faint, diffuse halo surrounds the bulge, with subtle extensions suggestive of a very faint disk component. There is little indication of strong spiral arm structures or other prominent features typically associated with actively star-forming galaxies. The color indices suggest a population of older stars, with a redder overall hue. There are also some small hints of merging or tidal debris, although the signs of disturbance are subtle, and any potential interaction with other galaxies seems to be minimal.
