The galaxy presents as an elongated, diffuse structure. The central region appears more concentrated, exhibiting a higher surface brightness. Proceeding outward from the core, the light attenuates, forming a less defined halo. There is a subtle asymmetry along its major axis, possibly indicative of tidal interactions or internal dust lanes. The color gradient suggests a mixed stellar population, potentially with older stars concentrated in the central bulge and younger, bluer stars in the outskirts. A faint, extended tail-like structure is visible on one side, suggesting a possible merger or interaction with another galaxy. A slight distortion to the overall shape is evident.
