The galaxy appears to be a relatively smooth, elliptical or lenticular galaxy, displaying a high degree of central concentration. There are no visible spiral arms or bar structures. The morphology is largely spheroidal.

The galaxy has a noticeable reddish-orange hue towards its center, which may indicate an older stellar population dominated by red giants and a lack of ongoing star formation in this region. Moving outwards from the core, the galaxy fades into a yellow/green coloration. This indicates a lack of large quantities of gas and dust.

There is no significant evidence of tidal features or morphological disturbances, suggesting it has not undergone a major merger recently. Any minor disturbances are likely to be unresolvable at this resolution.

Overall, the galaxy appears to be a mature, quiescent system.
