The galaxy presents a generally smooth morphology, with no immediately apparent spiral arm structure. The central bulge region exhibits a bright, concentrated luminosity, suggestive of a substantial stellar population and potentially an active galactic nucleus.

The overall shape appears to be somewhere between round and elongated, but leans more to the elongated. There is some suggestion of minor morphological disturbances; there may be faint tidal features or asymmetries indicative of past or ongoing interactions with other galaxies.

The galaxy displays a colour gradient, with the central regions exhibiting a more reddish-yellow hue, potentially indicating older stellar populations and/or significant dust obscuration. The outer regions are relatively bluer.
