The galaxy appears as a slightly elliptical, concentrated source of light with a dominant yellow-orange hue, indicating an older stellar population. It exhibits a largely smooth texture, though there is some visible irregularity in its structure. Dimmer, reddish patches are observed towards the periphery of the central light concentration, possibly indicating regions of ongoing, albeit subdued, star formation or dust obscuration. There is no clear evidence of a defined spiral arm structure or a prominent galactic disk. The galaxy does not appear to be significantly disturbed or undergoing a major merger event. A minor disturbance, such as a potential tidal interaction with a smaller companion, cannot be entirely ruled out based on the slight asymmetry. Overall, the galaxy presents as a relatively evolved system with a dominant spheroidal component.
