The galaxy presents as an elliptical morphology with a high degree of central concentration. The light profile appears smooth, lacking any obvious spiral arm structures or prominent dust lanes. Color gradients suggest a redder core region, indicative of an older stellar population. The overall form is generally rounded, exhibiting a mild degree of ellipticity, but appears to be more round than cigar shaped. There is no visual evidence of any major mergers or significant tidal disturbances within the immediate vicinity of the galaxy. Given the lack of visible features, the galaxy is likely undergoing a low rate of star formation.
