The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits an elliptical morphology, appearing mostly round with a slight elongation. The color profile suggests a dominant population of older stars, exhibiting a reddish hue. There appears to be a lack of substantial dust lanes or prominent spiral arm structures. There is no significant morphological disturbance visible, suggesting that it is likely not undergoing a major merging event. Star formation activity is present, but relatively low.
