The galaxy presents as a lenticular or elliptical type, exhibiting a smooth, concentrated light profile with a slight elongation. The central region displays a bright, compact core, indicative of a possible supermassive black hole or a dense stellar population. Moving outward from the core, the light gradually fades, showing a diffuse halo surrounding the central bulge. There's no discernible spiral arm structure or dust lanes visible in this image. It has a red hue and an estimated diameter of around 5 kpc. It appears relatively isolated, with no obvious signs of interaction or ongoing merger activity, although there are some minor disturbances. This suggests a relatively quiescent system with a low star formation rate. The galaxy's shape is slightly cigar-shaped, although overall, it appears primarily smooth.
