The galaxy presents as a centrally concentrated, smooth object with a generally elliptical morphology. There is a dominant, bright, yellowish-white core that appears nearly spherical. The light distribution diffuses outwards from the center, gradually fading into the background. Hints of a disk structure are apparent, with a subtle extension along the major axis. The disk exhibits a bluer hue compared to the central bulge. Overall, the galaxy displays a lack of significant spiral arm structure or prominent dust lanes, suggesting an older stellar population, and a relatively low star formation rate. There are hints of minor disturbances or interactions, but it appears to be an isolated object undergoing no major merging events.
