This galaxy presents a generally smooth morphology. The light distribution appears centrally concentrated, with a gradual decrease in intensity moving outwards from the core. The overall shape is elliptical, exhibiting a round form with a slight deviation towards an elongated, cigar-like appearance. There's no strong evidence of spiral arm structure or prominent disk features. The color is relatively uniform, with a subtle shift towards redder hues, suggesting a stellar population dominated by older, evolved stars, and low ongoing star formation. There are no obvious signs of recent or ongoing major merger events. Faint asymmetry, a slight warp, or tidal disturbance may exist, but it is not prominent.