The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with no discernible spiral arm structures or prominent dust lanes. Its shape is slightly elongated, deviating from a perfectly circular profile. The color gradient suggests a centrally concentrated population of older stars, appearing more yellow/orange, with a subtle shift toward bluer hues in the outer regions, indicating a younger stellar population might be present. There is no evidence of any major merger events or tidal disturbances. A potential small disturbance cannot be ruled out, as the galaxy shows a slightly irregular profile. The overall appearance points to a galaxy that is relatively quiescent in terms of star formation activity, although some minimal star formation may be present.
