The galaxy exhibits a smooth, centrally concentrated morphology. It appears elliptical in shape, with a slight elongation. The light is dominated by older stellar populations, exhibiting a yellowish to reddish hue. There is no evidence of distinct spiral arms or significant dust lanes. It displays an overall uniformity in color and texture. The galaxy appears relatively isolated, with no obvious signs of recent or ongoing major mergers. Minor disturbances may be present based on faint asymmetries. The estimated physical size suggests it is a moderately sized galaxy.
