The galaxy presents as a relatively smooth, elliptical-like structure. There is a concentrated central bulge that emits a yellowish-white light. The outer regions of the galaxy appear less defined, with a gradual decrease in light intensity suggesting an extended halo. The morphology suggests a lack of significant recent or ongoing merger activity. There is no discernible spiral arm structure or prominent dust lanes visible in this image. Based on the color profile, the galaxy appears to be a relatively evolved system, dominated by an older stellar population.
