The galaxy presents as a luminous elliptical morphology. The core exhibits a bright, concentrated glow, suggestive of a significant stellar population density. The radial light profile decreases smoothly from the center outwards, indicating a lack of distinct spiral arms or strong features. A slight elongation is observed, giving it a somewhat cigar-shaped appearance. The galaxy's outer regions show a subtle fading into the background, but appear relatively smooth and undisturbed, with little evidence of major tidal interactions or recent mergers. A minor asymmetry might be present, requiring further investigation to determine its origin. Colors indicate a substantial population of older stars, though a degree of ongoing star formation is likely.