The galaxy presents a generally smooth morphology, appearing elliptical in shape. It exhibits a concentrated central bulge that is relatively bright and has a slight reddish hue, suggesting an older stellar population. The galaxy displays a gradual decline in surface brightness from the center outwards. The overall color profile indicates a relatively quiescent state, with some evidence of ongoing star formation in the outer regions, as indicated by the slight bluish-green tint. There is no clear indication of spiral arms or significant dust lanes. Overall, the galaxy appears to be a massive system with a dominant spheroidal component. There is no clear indication of any major ongoing merger activity, though minor disturbances or interactions cannot be entirely ruled out.
