This galaxy appears to be a relatively smooth, elliptical or lenticular system. It exhibits a concentrated central bulge with a yellowish-white hue, suggesting an older stellar population. The outer regions of the galaxy fade gradually into a diffuse halo. The overall color gradient indicates a possible decrease in star formation activity from the core outwards. There's no clear evidence of spiral arms or significant dust lanes visible in this imaging. It appears somewhat elongated, but the light distribution is generally even and symmetrical. There are hints of a very faint disk, but this is difficult to see clearly.
