This galaxy appears to be an elliptical galaxy. It presents as a largely homogenous, smooth distribution of light, with minimal evidence of spiral arms or a distinct disk structure. It exhibits a concentrated central bulge with a gradual decrease in luminosity outwards, suggesting a relatively old stellar population. The color profile indicates a yellow/white core transitioning to a redder outer region, which may be indicative of older stars and diminished star formation in these peripheral areas. Overall, it appears to be a relaxed system with no major morphological disturbances or ongoing mergers. There is no evidence of a strong active galactic nucleus (AGN) from the image alone. The galaxy is approximately 3.3 kiloparsecs in diameter, which places it as a dwarf elliptical galaxy.