The galaxy presents as a single, luminous entity with a generally smooth morphology. Its overall form is somewhat rounded, exhibiting a subtle elongation that is neither perfectly spherical nor cigar-shaped. The light distribution suggests a centrally concentrated structure, with a gradual decrease in brightness towards the outer regions. The colour profile indicates a population of older stars, lacking a significant presence of active star formation. The galaxy appears relatively undisturbed, with no obvious signs of major ongoing or recent merger activity. A faint hint of irregularity may suggest a possible minor interaction or internal disturbance, however, further data are necessary for confirmation. Overall, it appears to be a relatively relaxed system without prominent features.
