The galaxy presents as a relatively smooth, elliptical-like structure. The light profile appears centrally concentrated with a gradual decrease in surface brightness moving outwards. The core region exhibits a yellowish hue, suggesting a population of older stars. There is some evidence of a faint, extended halo surrounding the main body. No prominent spiral arms or distinct dust lanes are discernible within the image. The overall morphology indicates a system that is likely dynamically evolved, potentially with ongoing, but not particularly intense, star formation activity. There is no evidence of a major ongoing merger or strong tidal disturbances, although subtle asymmetries cannot be entirely ruled out at this resolution.
