The galaxy presents a primarily smooth and elliptical morphology. The central region appears very bright and concentrated, indicating a significant stellar density, likely an old stellar population with minimal ongoing star formation. The galaxy is elongated, exhibiting an intermediate degree of roundness. There are no obvious spiral arm structures or features indicative of significant ongoing mergers or major disturbances, though a minor disturbance cannot be ruled out due to the faint outer regions of the disk. The color indices suggest the galaxy is composed of older stars with fewer young blue stars, possibly resulting in a relatively high mass and low current star formation rate. The size of the galaxy appears to be on the smaller size when compared to other galaxies. 