The galaxy presents as a moderately sized elliptical or lenticular galaxy, exhibiting a generally smooth and symmetrical morphology. The light distribution suggests a central bulge that dominates the overall structure, with a gradual decrease in luminosity towards the outer regions. There is no clear evidence of spiral arms or a distinct disk component. The color profile appears to be relatively uniform, displaying a yellowish-white hue, indicative of an older stellar population with minimal ongoing star formation. A slight elongation is noticeable, suggesting it is somewhere between being round and cigar shaped. Subtle disturbances may be present, but overall it does not appear to be undergoing a major merger.