The galaxy presents as a generally smooth, centrally concentrated object with a moderate degree of radial symmetry. The light distribution suggests an elliptical morphology. The central region exhibits a bright, yellowish-white core, indicative of a high density of older stellar populations. Moving outward from the core, the color transitions towards a slightly redder hue, likely indicating the presence of a mix of older stars and dust. There is no clear evidence of spiral arm structure, bar features, or significant dust lanes. The outer edges of the galaxy gradually fade into the background sky, suggesting a relatively smooth density profile. There are no indications of strong tidal distortions or major ongoing merger events. Faint disturbances could be present but not noticable in the image.
