The galaxy exhibits a generally elliptical morphology, displaying a smooth, centrally concentrated light distribution. The core appears bright and yellowish, suggesting a population of older stars. Moving outward from the core, the galaxy transitions to a slightly bluer hue, indicating the presence of some younger stars. The overall structure lacks distinct spiral arms or features, exhibiting a relatively homogenous texture, with some minor potential disturbances. There is a slight asymmetry present, though without a clear indication of an ongoing merger. The galaxy's apparent roundness suggests a low inclination angle relative to our line of sight.
