The galaxy presents as an elliptical morphology, exhibiting a smooth and largely featureless light distribution. It appears elongated, with a cigar-shaped structure. The central region exhibits a higher concentration of light intensity, gradually fading towards the outer edges. The color profile is predominantly redder, suggesting a population of older stars with minimal ongoing star formation. There is no obvious presence of spiral arms or a distinct disk structure. No apparent signs of major mergers or tidal disturbances are observed, although minor irregularities cannot be ruled out at this resolution.
