The galaxy presents as a generally smooth, elliptical structure. A concentrated, bright core is readily apparent, exhibiting a yellowish-orange hue. Moving outwards from the core, the galaxy's luminosity decreases gradually, maintaining a similar color profile but with a slight shift towards redder tones in the outer regions. There is little to no evidence of distinct spiral arms or significant dust lanes; the overall appearance is relatively featureless. The galaxy exhibits a slightly elongated shape, appearing more "in between" round and cigar-shaped, with no signs of any ongoing major mergers or significant tidal disturbances. The morphology suggests a relatively evolved system, potentially nearing the end of its star-forming lifecycle, characterized by an older stellar population.
