This galaxy appears to be a relatively compact system. It displays a generally smooth morphology, indicative of an elliptical or lenticular type. The color profile suggests a dominance of older stellar populations, as evidenced by the yellowish-red hue concentrated towards the central region. However, a slight blue tint is present in the central core of the galaxy. There are no apparent spiral arms or a distinct disk component.

Evidence of possible interaction or recent merger activity is suggested. The object is not completely symmetrical. It also exhibits an uneven distribution of light, with some regions appearing slightly more disturbed than others. The overall structure is dominated by a central bulge or core, which seems to be the brightest and most densely packed part of the galaxy.
