The galaxy appears as a centrally concentrated object with a relatively smooth morphology. Its color profile suggests an older stellar population, exhibiting a yellowish hue. There is a lack of distinct spiral arm structure or prominent dust lanes, indicating it may be an elliptical galaxy or a lenticular galaxy seen face-on. There is a faint, diffuse halo surrounding the central bulge, with no obvious signs of ongoing major mergers or significant tidal disturbances. The light distribution is fairly symmetrical, suggesting a relaxed dynamical state.
