The galaxy presents as a relatively smooth, elliptical morphology. There is a slight elongation, but it largely appears rounded. The central bulge exhibits a concentrated brightness profile, indicating a high density of stars. The overall color is skewed toward the redder end of the spectrum, suggesting an older stellar population and possibly diminished star formation activity. There are no visually distinct spiral arms or prominent dust lanes discernible within this image. Faint disturbances indicate possible prior or ongoing minor interactions with satellite galaxies, but it is generally an isolated system.
