The galaxy appears as a relatively compact, elliptical-like structure. It exhibits a smooth light distribution, with a high degree of central concentration. The color is a yellowish-red hue, indicative of a population of older stars. There is a faint indication of minor tidal disturbances in the form of a slight irregularity, suggesting past or ongoing gravitational interactions with smaller objects. The galaxy shows no obvious spiral arms, bars, or dust lanes, and there is no significant evidence of active star formation.
