The galaxy appears to be a relatively smooth, elliptical type, exhibiting a centrally concentrated bulge. The galaxy demonstrates a bright, yellowish hue, suggesting a population of older stars and a relatively low rate of ongoing star formation. The galaxy's light distribution is largely spheroidal, with a gradual decrease in brightness towards the outer regions. A slight elongation is visible, but the overall shape remains consistent with an elliptical classification. There appears to be a tidal tail present, suggesting a merger. The tail may indicate some interaction, either past or ongoing, with a smaller object.
