This galaxy presents as a roughly elliptical, though somewhat irregular, structure. The central region exhibits a brighter, more concentrated luminosity. The overall color appears to be bluish-white, suggesting a population of relatively young stars. The lack of distinct spiral arms, combined with the relatively smooth light distribution, indicates a morphology leaning towards an elliptical or lenticular classification.

There are suggestions of some minor disturbances in the outer regions of the galaxy, potentially due to ongoing or past interactions with other galaxies. It does not appear to be isolated, indicating potential influence from its surroundings.
