The galaxy presents an elliptical morphology, with a somewhat smooth overall appearance. The central bulge exhibits a yellow-orange hue, suggesting a population of older stars. Fainter, bluer regions are present in the outer regions of the galaxy, possibly indicating areas of more recent, albeit low-level, star formation. There is a slight asymmetry visible in the galaxy's outer regions, which could be indicative of a minor interaction or past merger event. No prominent spiral arm structure is observed, though a hint of a disk can be inferred from the flattening of the galaxy along a central axis. Overall, the galaxy appears to be in a relatively quiescent state, with ongoing, low-level star formation activity.
