The galaxy presents a slightly elongated, cigar-shaped morphology. The light distribution is generally smooth, with a diffuse appearance suggesting a dominant spheroidal component. There is faint evidence of a possible disk-like structure, however, it is subtle.

The galaxy exhibits a color gradient, appearing bluer towards the central region and gradually becoming redder towards the outer edges. Some asymmetries and slight disturbances are observable, suggesting possible tidal interactions with companion galaxies, however, no clear signs of merging events are immediately obvious. 
