The galaxy presents as a single, relatively compact object. Its overall morphology suggests a largely smooth structure, with little apparent evidence of spiral arms or significant disk features. The shape is generally rounded, lacking a pronounced elongation or cigar-like appearance. There is no immediately apparent indication of major mergers or significant tidal disturbances affecting the galaxy's morphology. The light distribution appears fairly even. The concentration of the galaxy's light suggests a central bulge or core region. The galaxy exhibits a reddish hue overall, hinting at a stellar population dominated by older, redder stars.
