The galaxy presents as a single, cohesive structure with a generally elliptical morphology. There is a smooth, diffuse appearance to the light distribution, suggesting a lack of prominent spiral arms or dust lanes. The central region exhibits a higher surface brightness, indicative of a bulge component. The color profile is suggestive of a stellar population that is transitioning from blue to red. The galaxy's structure appears undisturbed, without any obvious signs of recent major mergers or tidal interactions. A slight asymmetry can be observed in the outer regions, but is not obvious.