The galaxy presents a largely smooth, elliptical morphology. It exhibits a concentrated central bulge that appears bright and nearly spherical. Moving outward from the core, the light gradually diminishes into a diffuse halo. There are hints of faint, broad spiral arms, but these are not well-defined; the overall structure appears more lenticular. The color profile suggests an older stellar population, with a redder hue in the outer regions and a slightly bluer tint closer to the core. There's no significant evidence of active star formation observable in this image, implying a relatively quiescent galaxy. No signs of a major merger are readily apparent, however, a minor disturbance cannot be ruled out due to the potential fuzziness observed in the halo. The overall impression is that of a galaxy that is approaching a more stable, evolved state.