The galaxy appears as an elliptical or lenticular type, exhibiting a generally smooth and centrally concentrated luminosity profile. It presents an elongated shape, with the major axis significantly larger than the minor axis. There are no distinct spiral arm structures or prominent dust lanes visible in this image.

The central region displays a bright, concentrated core, potentially indicative of a supermassive black hole or dense stellar population. The color of the central region appears somewhat redder than the outer regions. The outer regions are fainter with a bluer color gradient, suggesting a population of younger stars.

There might be a very subtle minor tidal disturbance or asymmetry in the outer regions, but the main structure appears generally undisturbed and not undergoing any major merging event.
