The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. It exhibits a generally round morphology, with only a slight deviation from perfect circularity. There is minimal evidence of significant spiral arm structure or prominent dust lanes within the visible portion. The galaxy's color profile indicates a redder hue overall, suggestive of an older stellar population and relatively low ongoing star formation. There are no obvious signs of major mergers or tidal disturbances, although the galaxy's subtle asymmetry could potentially indicate a past minor interaction or disturbance event.
