The galaxy appears to be a relatively smooth and rounded system. It exhibits a concentrated central bulge that dominates its overall structure. A very faint and diffuse disk component may be present, but the resolution limits certainty. There is no apparent spiral arm structure or evidence of a recent major merger event. The galaxy's color is relatively uniform across its body, showing a yellowish hue indicative of a mature stellar population. The smooth morphology suggests that star formation rates are low, resulting in a galaxy dominated by older, redder stars. The overall structure suggests the galaxy is likely an elliptical or S0 type.
