The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity profile, suggesting a high density of stars. There is a slight elongation to the galaxy's overall shape, though it is primarily round. A possible minor disturbance or companion is visible as a redder and less-luminous region to the upper left of the main body, potentially indicating a past or ongoing interaction. The galaxy displays a yellow/orange hue, indicative of an older stellar population and lower star formation activity. No distinct spiral arms or significant dust lanes are discernible. There is no strong evidence of an actively merging system.
