The galaxy presents as a relatively compact, luminous object with a distinct central bulge that dominates the overall morphology. The color profile suggests an evolved stellar population, exhibiting a yellowish-red hue consistent with older stars. There appears to be a faint, diffuse halo or extended stellar envelope surrounding the primary body of the galaxy.

Morphological features hint at possible past or ongoing gravitational interactions. A faint tidal tail or plume-like structure seems to extend from the main galactic body, which could indicate a minor merger event. Disturbances may exist within the galactic disk, causing non-symmetric features. This is based on the irregular shape of the galaxy. Star formation appears to be low to moderate based on the yellowish color.
