The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. There are no apparent spiral arms or significant dust lanes visible in this image, implying a lack of ongoing major star formation. The galaxy exhibits a flattened shape, appearing somewhere between round and cigar-shaped. A slight asymmetry may suggest minor gravitational interaction or disturbance, although the overall structure is generally undisturbed, with no large merging or tidal features detected. Its color is primarily reddish, indicating an older stellar population. The estimated effective radius suggests that the galaxy possesses a significant physical size. Low star formation rates may be due to the galaxy's stage of evolution, possibly representing an early type galaxy where star formation has slowed down.
