The galaxy presents an overall elliptical morphology, though it appears somewhat disturbed. A prominent central bulge exhibits a bright, yellowish-white hue, suggesting a population of older stars. Extending outwards from this bulge is a fainter, bluish disk component. The disk appears asymmetrical, potentially indicating ongoing or past gravitational interactions. Patches of reddish light are visible, possibly indicative of regions with significant dust obscuration or HII regions associated with active star formation. Overall, the galaxy appears to be undergoing some form of evolutionary process, with the smooth central bulge contrasting with the more chaotic structure of the disk.
