The galaxy presents a largely smooth morphology, appearing as a centrally concentrated elliptical or lenticular type. Its overall shape is notably round. There is no obvious disk structure, nor are there prominent spiral arms visible. The central region exhibits a high luminosity, with a gradual decrease in brightness towards the outer edges, suggesting a relatively uniform stellar population or the presence of a featureless disk. There are no apparent signs of ongoing major mergers or significant tidal disturbances. The overall color index suggests a population of older, redder stars. The galaxy's size appears to be moderate within the observed field.
