The galaxy presents as a relatively smooth, elliptical structure. Its central region exhibits a high degree of luminosity, appearing almost spherical with a yellow-white hue, indicative of a population of older stars. Fainter, diffuse extensions are visible around the core, contributing to the overall elliptical shape. These extensions have a redder color, possibly due to dust obscuration or a population of older, redder stars in the outer regions. The major axis is oriented approximately NW-SE. No distinct spiral arms or prominent dust lanes are observed, suggesting it is most likely an early-type galaxy. There appears to be no active galactic nucleus, based on the consistent coloration and lack of a concentrated point source.
