The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated bulge region, with a gradual decrease in luminosity outward from the core. The galaxy's overall shape appears slightly elongated, but is mostly close to being round. There is evidence of a faint, extended halo surrounding the main body of the galaxy, though the image resolution limits detailed assessment. Colors suggest a stellar population dominated by older stars, primarily residing in the bulge, with a small presence of younger stars located in the outer regions of the galaxy. Evident is a low level of ongoing star formation within this system. There is no indication of any significant disturbance or ongoing mergers with other galaxies.
