The galaxy presents a generally smooth morphology, with an overall elliptical appearance. The light distribution appears centrally concentrated, with a gradual decrease in surface brightness moving outwards from the core. There is a slight elongation, with the galaxy's shape being more 'in-between' round and cigar shaped. There is no obvious spiral arm structure or prominent dust lanes visible, suggesting a lack of significant disk component. Its color is primarily yellow to white, indicative of an older stellar population with fewer young, massive stars. There is no strong evidence of ongoing major merger activity, though some minor disturbance cannot be ruled out given the image quality. The galaxy is relatively compact, with its light concentrated in a small region.
