The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile shifts from a yellowish-white core to a more reddish and diffuse halo. There is very little observable disk or spiral arm structure, with only the slightest hint of asymmetry. The general smooth appearance suggests an older stellar population. The color gradient suggests some level of ongoing, albeit low, star formation within the central region. Overall, the galaxy appears to be relatively undisturbed, showing little evidence of recent merger activity. The light distribution is compact, corresponding to a small physical size for a galaxy at its distance.
