The galaxy presents a smooth, largely featureless morphology. It appears elliptical in shape, exhibiting a high degree of central concentration with decreasing luminosity outwards. The central region is a bright, yellowish hue, suggesting an older stellar population likely dominating the core. The outer regions show hints of a redder tint, also consistent with older stars and a diminishing presence of younger, bluer stars characteristic of active star formation. There is no visible evidence of spiral arms, bars, or significant dust lanes. No signs of any major ongoing merger events or tidal disturbances are observed. Overall, the galaxy seems to be a relatively quiescent system dominated by an evolved stellar population.
