The galaxy presents as a relatively smooth, elliptical-like structure with a dominant central bulge. The overall color profile suggests a population of older stars, leaning towards redder hues with some hints of yellow. There is no clear evidence of spiral arms or significant dust lanes. The galaxy appears well-defined, with a noticeable concentration of light towards the center. The outer edges of the galaxy gradually fade into the background, indicating a smooth density profile. No signs of major disturbances or ongoing mergers are immediately apparent, suggesting a relatively settled morphology. Overall, the galaxy exhibits characteristics consistent with an evolved system with limited ongoing star formation.
