The galaxy presents as a relatively smooth, elliptical form. The light distribution suggests a centrally concentrated spheroid with a bright nucleus. The galaxy exhibits a subtle color gradient, transitioning from a bluer core to redder outer regions. There is no obvious evidence of spiral arms or a prominent disk structure. The galaxy appears to be in a relatively undisturbed state, with no significant tidal features or signs of a recent major merger evident in the immediate vicinity. The overall morphology suggests a system dominated by older stellar populations, with little ongoing or recent significant star formation activity. The shape is moderately elongated, with a cigar-like appearance. It seems to have been classified as a non-merging galaxy.
