The galaxy presents as a largely smooth, elliptical structure. It exhibits a distinct central bulge, characterized by a concentrated brightness gradient. The overall color profile suggests an older stellar population, with a redder hue in the central regions, grading outward to slightly bluer tones in the outer halo. There is little to no visible evidence of spiral arms or significant dust lanes. The galaxy appears to be relatively isolated, showing no strong signs of tidal interactions or ongoing mergers, although subtle distortions in the outer isophotes cannot be ruled out without higher resolution imaging. The shape is generally rounded, tending toward elliptical rather than a highly elongated or irregular form. Overall, the morphological features align with those of an early-type galaxy, possibly an elliptical or lenticular galaxy at a moderate distance.
