The galaxy presents as a centrally concentrated, smooth elliptical-like system. It appears largely featureless, lacking significant spiral arm structure or prominent dust lanes. The light distribution is centrally concentrated, with a noticeable, smooth decline in brightness towards the outer regions. There is a slight elongation in the overall shape, hinting at a possible deviation from a perfect sphere. The color is somewhat yellow-red, indicating the presence of an older stellar population and/or dust obscuration, which indicates a lower star formation rate. There is no evidence of ongoing major merging activity or significant tidal distortions, but possibly some minor disturbance. The overall morphology suggests a galaxy that is likely a relatively evolved system.
