The galaxy presents an overall elliptical morphology. It is elongated, appearing cigar-shaped rather than perfectly round. The central region exhibits a bright, concentrated bulge, possibly indicative of an older stellar population. Moving outwards from the core, a faint, diffuse disk is suggested with some irregularities visible. These irregularities could be indicative of tidal interactions or disturbances, and there may be a possibility of an ongoing merger or recent merger event. The color gradient transitions from a yellow/orange hue in the core to a slightly bluer tint in the outer regions, possibly suggesting a higher rate of star formation in those regions. The overall structure shows evidence of both smooth, featureless components and disturbed components.
