The galaxy presents an elliptical morphology, appearing relatively smooth and concentrated toward the center. The light profile suggests a high degree of central concentration, with the majority of the luminosity originating from a bright core region. There is little evidence of spiral arm structure or significant dust lanes. The galaxy's color is generally yellow/orange, indicating an older stellar population. There are hints of bluer regions located on the outer edges of the galaxy, but it appears fairly subdued. There is no clear indication of ongoing major merging activity or strong tidal disturbances in the galaxy’s structure, although there is some possible asymmetry that could be a result of minor disturbance.
