The galaxy appears to be an elliptical galaxy, exhibiting a smooth, diffuse light profile. It presents a somewhat elongated shape, with the major axis extending approximately twice the length of the minor axis. The central region is significantly brighter, indicative of a dense stellar population, likely an older population given the lack of discernible blue light. There is no obvious spiral arm structure or dust lane features, further supporting the elliptical classification. The overall color suggests a redder population of stars, consistent with a galaxy where star formation is minimal or has ceased altogether. Small disturbances in the elliptical shape suggest a past minor merging event.
