The galaxy presents as a relatively smooth, centrally concentrated object. Its overall shape is elliptical, appearing moderately flattened rather than perfectly spherical or highly elongated. The central bulge is prominent and exhibits a bright, yellowish hue suggesting a population of older stars. Moving outward from the core, the light gradually fades into a more diffuse halo. There is little evidence of spiral arm structures or significant dust lanes, although subtle variations in color might imply some level of substructure. Overall, the object appears to be an elliptical galaxy with signs of only minor past or present interactions.
