The galaxy presents an elliptical morphology, exhibiting a smooth light distribution with no discernible spiral arms or bar structures. The core region is bright and concentrated, suggesting a high stellar density, possibly indicative of an aged stellar population. The galaxy displays a color gradient, transitioning from a yellowish-white core to a redder hue in the outer regions. This color variation may reflect differences in stellar population age, metallicity, or dust content, with potentially older and/or more metal-rich stars dominating the central bulge and younger, bluer stars sparsely distributed in the outer regions. There are slight asymmetries, but no prominent tidal tails or other signatures of recent major mergers are apparent.
