The galaxy presents a generally smooth and centrally concentrated morphology. It exhibits an elliptical shape, appearing somewhat elongated but not significantly cigar-shaped. The light distribution suggests a dominant bulge component with a radial profile that fades gradually into the surrounding halo. There is no visible evidence of spiral arms or significant dust lanes. The galaxy's color is predominantly yellowish, which indicates an older stellar population with relatively low levels of ongoing star formation. There is no evidence of recent major merger activity or strong tidal disturbances, although some minor irregularity cannot be entirely ruled out. The galaxy's overall structure suggests a relatively evolved system.
