The galaxy appears to be a relatively smooth, elliptical or lenticular system. Its overall form is round and symmetrical, with no obvious spiral arm structure or bar features visible. The central bulge region is bright and concentrated, exhibiting a yellowish hue, suggesting an older stellar population. Moving outward from the core, the galaxy fades gradually, indicating a diffuse halo. There may be some subtle irregularities in the outer regions, suggestive of past interactions or minor disturbances, however they appear to be minimal. The overall color profile indicates a population of evolved stars and a relatively low rate of current star formation.
