The galaxy presents as a moderately bright, elliptical or lenticular system. Its morphology appears largely smooth, with a high concentration of light towards the center. There is a suggestion of a slight flattening, tending towards an oblate spheroid shape rather than a perfectly circular profile. A subtle color gradient can be observed, with the central region exhibiting a more yellowish hue, potentially indicative of an older stellar population, while the outer regions appear marginally bluer, suggestive of some ongoing, though likely subdued, star formation. No prominent spiral arms, bars, or other distinct features are discernible. There is no evidence of any major ongoing mergers or interactions, though very minor disturbances cannot be ruled out. Overall, this galaxy seems to be a fairly evolved system, with the bulk of its stellar mass already in place.
