The galaxy presents a largely smooth, elliptical morphology. It appears nearly circular in shape, exhibiting minimal flattening. The light distribution suggests a centrally concentrated luminosity profile, with a bright, relatively small core that gradually diffuses outward into a fainter, more extended halo. There are no distinct spiral arms or prominent dust lanes visible. There appears to be a slight color gradient, with the central region appearing somewhat bluer than the outer halo, which trends towards redder hues. There is no visual evidence of any ongoing major merging activity or significant tidal disturbances.
