The galaxy presents as an elliptical or lenticular type, exhibiting a smooth, concentrated luminosity profile. The central bulge is prominent and appears significantly brighter than the surrounding galactic disk. The galaxy's overall shape is elongated with an axis ratio indicating a moderate degree of ellipticity, deviating somewhat from a perfect sphere.

There is little evidence of distinct spiral arm structures or significant dust lanes. The color appears generally redder across the galaxy, which suggests a stellar population dominated by older, redder stars with limited ongoing star formation. Subtle color variations exist within the galaxy, but these are minimal. The disk, though present, lacks the distinct features and vibrant star-forming regions typically observed in spiral galaxies. There is a faint suggestion of possible tidal disturbances or minor interactions.
