The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a dominant bulge and a flattened disk component. The bulge region shows a concentrated, luminous intensity. The disk shows an overall smooth light distribution, with no obvious spiral arm structure immediately visible at this resolution. It is likely that the disk is comprised primarily of older stellar populations.

There is a suggestion of color gradient within the galaxy, where the central bulge exhibits a redder color. This could be indicative of an older, more metal-rich stellar population concentrated within the bulge. The outer disk shows a subtle bluer tint, suggesting the presence of younger stars or regions of recent star formation, even if faint. There is no evidence of a ongoing major merger event. Overall, the galaxy appears relatively undisturbed.
