The galaxy presents an elliptical morphology, with a cigar-shaped appearance. The central region exhibits a high concentration of light, suggesting the presence of an older stellar population. The color profile is generally redder overall, transitioning to slightly bluer hues further from the central bulge. There are no significant spiral arm structures or dust lanes readily apparent. The galaxy appears relatively smooth, with only minor signs of disturbance in its overall structure and no clear evidence of a recent major merger event. The overall size is relatively compact. The estimated mass appears substantial. Though the star formation rate is rather low, there is still activity in the galaxy.
