This galaxy appears to be a relatively smooth, elliptical type. The light is concentrated towards the center, indicating a bulge structure. The galaxy exhibits a yellowish-red hue, which suggests an older stellar population dominating its composition. There is minimal evidence of distinct spiral arms or significant dust lanes. The overall morphology suggests that the galaxy is generally undisturbed, without major signs of ongoing mergers or tidal interactions. The round shape may imply it lacks substantial rotational support. The relatively uniform color further supports the notion of a passively evolving system with low current star formation activity.