This galaxy appears to be a relatively smooth, elliptical galaxy with a notable lack of distinct spiral arm structure. It exhibits a generally spheroidal shape, with a high degree of roundness. The light distribution is concentrated towards the center, indicating a prominent galactic nucleus or core. The color profile suggests a population of older stars, based on its redder overall hue, but the magnitude suggests the existence of some young stars. There is some suggestion of a possible minor disturbance, like a smaller galaxy tidally interacting with the primary object, or other non-symmetric components. The overall structure does not appear to be undergoing a major merger event. The estimated size indicates that it is a substantial galaxy.
