The galaxy appears as a centrally concentrated object with a generally smooth morphology. There is an elliptical shape to the light distribution, but it is generally round. The galaxy exhibits a prominent central bulge with a color gradient towards yellower hues. The outer regions appear fainter with redder tones, and there is no evidence of spiral arm structure or prominent dust lanes. The overall structure suggests the galaxy may be an elliptical galaxy or a lenticular galaxy with a dominant bulge. There is no apparent indication of any recent or ongoing major merger events or significant tidal disturbances.
