The galaxy appears to be a relatively luminous elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. The core exhibits a bright, yellowish hue, suggesting an older stellar population. The overall shape deviates from a perfect circle, appearing slightly elongated. Faint, diffuse outer regions extend beyond the bright core, indicating a substantial halo component. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy appears relatively undisturbed, lacking any major signs of recent mergers or tidal interactions, though some minor disturbances cannot be ruled out at this resolution. Low levels of star formation may be occurring within the galaxy.
