The galaxy presents as an elliptical morphology, elongated along its major axis. The light distribution appears relatively smooth, exhibiting a centrally concentrated brightness profile that gradually fades towards the outer regions. A slight color gradient is discernible, transitioning from a bluer central region to redder hues in the outskirts, although the image quality limits a more in depth examination. There is no indication of spiral arms or distinct disk-like structures, nor any strong tidal features that would indicate a recent major merger event. The overall appearance suggests a galaxy dominated by an older stellar population, with a relatively low ongoing star formation rate. There is a slight asymmetry in the central region, suggesting minor disturbances, possibly a smaller merger.
