The galaxy presents as a relatively smooth, centrally concentrated object. The core exhibits a bright, somewhat diffuse glow, suggesting a significant population of older stars. The overall shape is elliptical, appearing mostly round. No obvious spiral arm structures are discernible. There's a very slight elongation or irregularity in the outer regions, hinting at a potential minor disturbance or interaction. The color profile indicates a redder core region transitioning to a bluer halo, suggesting a gradient in stellar populations and potentially, ongoing star formation in the outer regions. The light distribution is consistent with an early-type galaxy, likely an elliptical.
