The galaxy presents as a moderately bright, elliptical structure, with an apparent high degree of central concentration. Its overall shape is somewhat elongated, with the major axis oriented in a northwest-southeast direction. The light profile appears smooth with no prominent spiral arms or bar structures visible. The galaxy exhibits a strong central bulge, with its color indicating an older stellar population. Fainter, diffuse emission extends outwards from the bulge, suggesting a relatively large halo or extended stellar distribution. There are subtle hints of irregularities in the outer regions, potentially indicating tidal interactions or past merger events, though no distinct tidal tails or shells are readily apparent in the image.
