This galaxy presents as a roughly elliptical structure with a bright, concentrated central bulge. The light distribution appears smooth and relatively featureless, lacking distinct spiral arms or prominent dust lanes. The central region exhibits a yellowish-white hue, suggestive of an older stellar population, while the outer regions possess a bluer tint, hinting at some ongoing star formation. The galaxy appears to be somewhat elongated, rather than perfectly spherical. There is no indication of any major mergers or significant tidal disturbances affecting the morphology of the galaxy. The overall light profile suggests a relatively relaxed and evolved system.
