The galaxy presents as a relatively compact object, approximately elliptical in shape. A dominant, centrally concentrated bulge is apparent, exhibiting a smooth, symmetrical morphology. The central region is characterized by strong emission across the green, red and z bands suggesting it may have active star formation. There is very little visual evidence of distinct spiral arms or significant disk structure. The galaxy appears moderately isolated, showing no obvious signs of major ongoing mergers or tidal interactions with neighboring galaxies, however there is evidence of minor disturbance within the bulge. The light distribution is relatively smooth and centrally concentrated, with a marked decrease in intensity toward the outer regions of the galaxy. Overall, it appears to be a relatively evolved galaxy with a moderately suppressed star formation rate.
