The galaxy presents a predominantly smooth morphology, suggesting it is likely an elliptical galaxy or a lenticular galaxy viewed face-on. A diffuse, roughly elliptical halo surrounds a brighter, more concentrated central region. The galaxy exhibits a yellowish hue, indicative of an older stellar population with relatively little ongoing star formation. The overall shape appears largely undisturbed, showing no clear signs of major mergers or tidal interactions. There is a very slight irregularity on one side of the halo, which may indicate a minor disturbance or ongoing accretion event. The concentration of light is highest in the central core, gradually fading outwards into the more diffuse halo. There is minimal evidence of spiral arms or prominent dust lanes.
