The galaxy presents an elliptical morphology, with a moderate degree of flattening. The light distribution appears concentrated towards the center, indicating a prominent bulge component. The color gradient suggests a relatively older stellar population dominating the central regions, with bluer hues appearing in the outer regions. There are subtle irregularities in the outer regions, possibly indicating tidal disturbances or ongoing interactions. The galaxy's overall structure suggests a classification between a lenticular and an elliptical type, displaying characteristics of both.
