The galaxy presents as a relatively compact structure, exhibiting a smooth, somewhat elliptical morphology. A concentrated central bulge is observed, gradually fading into the surrounding halo. Faint, diffuse disk-like features may be present, although their exact structure is difficult to resolve. The galaxy appears to be yellow-white suggesting an older stellar population. There is no indication of strong ongoing star formation or significant dust lanes. Slight disturbances, possibly related to a minor interaction, may be present. No tidal tails or dramatic distortions are evident.
