The galaxy presents as an elliptical or lenticular system, appearing largely smooth with minimal discernible substructure. The central bulge exhibits high luminosity, indicative of a concentrated stellar population likely dominated by older, redder stars. Moving outwards, the galaxy shows a gradual decrease in surface brightness, with a faint, diffuse halo extending beyond the brighter core region. The overall shape approximates a slightly flattened spheroid, being in between round and elongated, with no obvious spiral arms or bar structures. No significant tidal features or signs of ongoing major mergers are apparent in the image, suggesting a relatively quiescent evolutionary state. Faint hints of a disk-like component may be present, based on a subtle color change away from the core, however the limited resolution prevents definitive classification.
