The galaxy presents as an elliptical or lenticular morphology, exhibiting a generally smooth light distribution with no discernible spiral arm structure. The central region displays a concentrated luminosity, suggesting a prominent galactic nucleus. There is a distinct lack of dust lanes or other features indicative of ongoing major star formation. The overall color profile appears relatively red, hinting towards an older stellar population with minimal recent star formation activity. The observed round shape, instead of a more elongated appearance, suggests that it is potentially viewed nearly face-on. Faint extensions of light surround the primary body of the galaxy, possibly indicating the presence of a diffuse halo. There is no evidence of tidal tails or distortions indicative of recent major mergers or interactions, though subtle disturbances may be present.
