The galaxy presents as a relatively smooth, elliptical-like object, with an apparent lack of significant spiral arm structure. It displays a concentrated central bulge with a noticeable decrease in surface brightness moving outward toward its undefined edges. The overall color appears to be redder, suggesting an older stellar population, with a distinct yellow-orange hue and indicating lower rates of recent star formation. There appears to be some asymmetry in the surface brightness distribution, potentially indicating some sort of minor interaction.
