The galaxy presents as a generally smooth, elliptical-like object with a high degree of central concentration. The galaxy exhibits a noticeable elongation, suggesting a possible transition between a more spherical and a lenticular morphology. The color profile indicates a dominant population of older stars, with a yellow-reddish hue particularly pronounced in the central region, suggesting minimal current star formation. While the overall structure appears relatively undisturbed, there is a subtle asymmetry, possibly indicative of minor gravitational interactions. The galaxy displays a substantial mass content.
