The galaxy presents as a relatively compact object, appearing smooth in texture with a slightly elliptical morphology. There is some indication of a possible minor disturbance to the galaxy's structure, but it is difficult to determine conclusively from the image alone whether this is due to a minor interaction or internal processes. The galaxy exhibits a color gradient, appearing bluer in the central regions, suggesting ongoing star formation. The outer regions show hints of older stellar populations. There is no clear indication of a strong tidal tail or major merger event. The galaxy's overall light profile seems to be dominated by a spheroidal component.
