The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a yellow-orange hue, suggesting a stellar population dominated by older, redder stars. There appears to be little evidence of spiral arms or significant dust lanes. The galaxy's overall morphology appears regular with no obvious signs of recent major mergers or tidal disturbances, though there may be a slight disturbance. The galaxy is estimated to be very massive with a very low rate of star formation. The shape is in between round and cigar-shaped.
