The galaxy presents as a primarily smooth, elliptical-like structure. Its shape appears somewhat elongated or cigar-shaped, lacking any distinct spiral arm features. The central region exhibits a concentrated, brighter luminosity, indicative of a significant stellar population. A gradual decrease in luminosity is observed extending outwards from the center towards the edges of the galaxy, creating a fuzzy or diffuse halo-like appearance. The overall color profile suggests a population dominated by older stars, possibly with ongoing star formation indicated by the object's color. There is no obvious visual evidence of any major mergers or significant tidal disturbances affecting the galaxy’s morphology. The object's form is largely undisturbed.
