The galaxy presents as a relatively smooth, elliptical structure with a high degree of central concentration. Its overall shape is predominantly round, exhibiting a nearly spherical morphology with minimal discernible features or disk-like components. The light distribution is smooth and diffuse, with a gradual decrease in intensity from the core outwards. There is no clear evidence of spiral arms, bar structures, or prominent dust lanes. There appears to be no major ongoing merger event, but subtle disturbances may be present based on the slightly irregular outer isophotes. The galaxy exhibits a yellowish-red color, suggesting an older stellar population.
