The galaxy appears as a somewhat rounded, singular object. Its light is centrally concentrated, with a diffuse halo extending outwards. The color profile suggests a mix of stellar populations; the core region exhibits a yellowish-white hue, potentially indicating older stars, while the outer regions show hints of bluer light, which could be attributed to younger, hotter stars or ongoing star formation. There is no clear indication of spiral arms or a defined disk structure. The galaxy's overall appearance suggests a relatively smooth morphology. There are no obvious signs of any major merger events or tidal disturbances.
