The galaxy presents a generally smooth and elliptical morphology. It appears largely featureless, lacking prominent spiral arms or a well-defined disk structure. The galaxy exhibits a concentrated central bulge that emits strongly. There is a gradual decrease in luminosity from the core towards the outer regions with no sharp boundaries observed, suggesting a smooth distribution of stellar populations. Its ellipticity is slightly elongated, showing it is not perfectly circular. There is no visual evidence of any major merging events or significant tidal disturbances, although there is a hint of a slight disturbance, which may represent a minor interaction with a smaller galaxy, or perhaps a tidal stream. Color gradients suggest potentially differing stellar populations, with the core appearing yellower than the outer regions, possibly indicating an older stellar population at the center. The estimated size suggests that this is likely a relatively large galaxy. Based on its colors, there is some star formation occurring, but not at a significant rate.
