The galaxy presents a generally smooth and elliptical morphology. There is a concentrated central bulge exhibiting a yellowish hue, indicating a population of older stars. The outer regions of the galaxy fade gradually, showing a subtle blue tint, potentially indicative of a younger stellar population or ongoing star formation, albeit at a relatively low rate. No distinct spiral arm structures or prominent dust lanes are discernible in this image. The overall appearance suggests a mature galaxy with a relatively quiescent star formation history. There is no apparent evidence of any major ongoing merging activity or significant tidal disturbances. The galaxy appears largely undisturbed and relaxed.
