The galaxy presents a roughly elliptical morphology, exhibiting a centrally concentrated luminosity profile that gradually diminishes towards the outer edges. The overall color of the galaxy appears slightly redder at the core, shifting to a bluer hue in the extended disk. This gradient potentially indicates a varying stellar population distribution, with older, redder stars dominating the central bulge and younger, bluer stars residing in the disk.

A slight asymmetry is observed in the galaxy's structure, potentially suggesting a minor gravitational interaction or disturbance. No distinct spiral arm structures are clearly resolved, possibly due to limitations in image resolution or intrinsic properties of the galaxy itself. The galaxy appears to be relatively isolated, without obvious signs of a major ongoing merger event. There is some subtle clumping on one side of the disk that could be suggestive of ongoing star formation or the remnants of a tidal interaction.
