The galaxy presents as a somewhat symmetrical structure with a concentrated central bulge. The galaxy's overall color profile skews toward the redder end of the spectrum, especially within the central region, indicating an older stellar population. The surrounding disk appears relatively smooth and lacking in significant distinct features such as prominent spiral arms or intense star-forming regions. There is a hint of a flattened disk-like structure with a slight ellipticity. Some minor irregularities and faint disturbances are suggested in the outer regions of the disk, potentially hinting at tidal interactions or recent minor merger events, however, these could be internal effects.
