The galaxy presents as a largely spheroidal object. Its central region exhibits a bright, concentrated core, implying a high density of stars in this area. Moving outwards from the center, the light intensity gradually diminishes, suggesting a smooth transition in stellar population density. The galaxy's overall color appears yellowish-orange. This color, combined with the smooth texture, may be indicative of a population of older stars. There is no readily apparent disk structure or spiral arm morphology. No prominent dust lanes or distinct star-forming regions are observable within the galaxy's structure. Overall, it presents the characteristics of an elliptical galaxy. There is some slight elongation evident, so it is not perfectly circular. There also appears to be some kind of disturbance on the right-hand side of the galaxy in the image. This may be due to some kind of tidal interaction with another, smaller, galaxy.
