The galaxy presents as a slightly elongated, lenticular-shaped structure with a smooth, diffuse appearance. There is a pronounced color gradient, transitioning from a predominantly reddish central region to greenish hues towards the outer edges. This suggests a differential distribution of stellar populations or dust content, with potentially older, redder stars concentrated in the core and relatively younger, bluer stars in the periphery. There is little evidence of defined spiral arms or prominent dust lanes. The overall morphology indicates a relatively evolved system with a potentially low rate of ongoing star formation. There are slight irregularities present in the outer structure suggesting possible past interactions with another galaxy, though these do not appear to be ongoing.
