The galaxy presents a generally smooth morphology. The primary structure appears largely spheroidal in shape but may be in the process of losing this quality. The light distribution appears concentrated, with a high degree of radial symmetry. The object displays a color gradient, transitioning from a bluer hue in the central region to a redder hue in the outer regions. There appears to be some distortion in the disk structure, potentially indicative of a minor gravitational interaction or disturbance. The object does not appear to be isolated, with hints of other objects near its edges that may or may not be related to the galaxy through tidal processes. Overall, the object appears to be undergoing some form of interaction that is altering its structure. Further investigation is needed to determine if the changes are caused by a merger event or something else.
