The galaxy presents as a centrally concentrated object, approximately round in appearance. A dominant, smooth spheroid component is evident. There is little to no discernible disk structure or spiral arm morphology. Faint features or subtle disturbances could be present, but not enough to determine any major merger events. The light distribution is relatively uniform, with no bright knots or HII regions readily apparent, suggesting a limited amount of star formation activity. The color index, judging by the redder hue, suggests a population dominated by older stars and/or significant dust reddening. Overall, the galaxy appears as a fairly evolved, massive system with a moderate red shift.
