The galaxy presents a generally smooth and round morphology, with a bright central bulge region exhibiting a yellowish hue, suggesting an older stellar population. There is a noticeable fainter, similarly colored region extending outwards and offset from the central bulge; it is unclear if this offset is a real structure of the galaxy or the result of image artifacts. The galaxy shows no strong evidence of spiral arms or significant disk-like structures within the optical wavelengths captured. The general color profile suggests a moderately evolved system undergoing some form of star formation. There may be signs of tidal disruption or a merging event. 
