The galaxy presents a morphology consistent with an elliptical or lenticular type, exhibiting a generally smooth light distribution across its main body. Its shape is largely round, although with a slight elongation suggesting a minor deviation from perfect circularity. 

There's potential evidence of interaction or merging activity. The primary galactic body has a somewhat disturbed appearance, with a possible secondary component or tidal feature extending from it. This could indicate an ongoing or recent merger event involving a smaller companion galaxy.

Color-wise, the galaxy exhibits a reddish-yellow hue, especially concentrated toward the central regions. This implies a stellar population that is largely old and metal-rich, with relatively little ongoing star formation. The tidal feature, if real, also shares this reddish color, further supporting the presence of an older stellar population within this structure.