The galaxy presents a largely featureless, smooth morphology, suggesting an elliptical classification. The light distribution is concentrated towards the center, exhibiting a high degree of central brightness. The overall shape appears mostly round, with no significant elongation or asymmetry apparent. There is little to no evidence of spiral arms, bars, or prominent dust lanes. The color profile indicates a population of older stars, exhibiting a redder hue in the central region, with a bluer distribution in the outer regions. There is no clear sign of any major ongoing merging activity or strong tidal disturbances affecting the system. Based on these characteristics, this galaxy is potentially a high-mass elliptical galaxy with a relatively low star formation rate.
