The galaxy presents as a relatively compact structure. It appears to exhibit a smooth morphology, with a dominant central bulge. There's an indication of a faint disk component, although any spiral arm structure is not clearly defined. The light profile suggests that this galaxy is fairly red, potentially indicating an older stellar population and/or significant dust obscuration. There are some signs of possible minor disturbances in its form, but it is likely a fairly relaxed system, and there is no obvious evidence of a major merger event. 
