The galaxy presents a primarily elliptical morphology, although there is some disk like structure. The central bulge is prominent, displaying a yellowish-white hue, suggestive of an older stellar population and a lack of ongoing star formation within this region. Surrounding the bulge, a bluish disk-like component can be observed. This blue coloration is indicative of younger, hotter stars, implying recent or ongoing star formation in the disk.

The galaxy appears to have a relatively smooth overall texture, although there are some irregularities and subtle distortions noticeable in the outer regions of the disk. These features could indicate minor gravitational interactions with another galaxy or perhaps internal disturbances. There is a suggestion of faint tidal tails or extended structures which may be indicative of interaction history. Overall, the galaxy appears to be in a relatively quiescent state, with moderate star formation activity mostly confined to the disk.
