This galaxy presents a relatively smooth, elliptical morphology, lacking prominent spiral arm structures. It exhibits a somewhat elongated shape, appearing as a cigar-shaped distribution of light. The light profile is centrally concentrated, with a gradual decrease in intensity outwards from the core. There is no clear evidence of ongoing major merger activity or significant tidal disturbances. Faint star formation might be present. The overall color suggests a population of older stars dominating the light output. The galaxy appears to be a relatively evolved system, likely residing at a moderate redshift.