The galaxy presents as a somewhat elongated, lenticular-like structure. The central bulge appears bright and concentrated, exhibiting a smooth texture and a dominant blue hue. This suggests the presence of a population of relatively young, hot stars within the bulge. Moving outward from the center, the galaxy displays a fainter, more diffuse disk. The disk lacks distinct spiral arms and has a generally smooth appearance. The redder areas in the outskirts suggest regions with older stellar populations or dust obscuration. There is some subtle evidence of possible tidal disturbance or faint interaction with another galaxy, however, the tidal features are very minor. Overall, this galaxy seems to be an intermediate mass galaxy with a relatively low rate of star formation.
