The galaxy presents as a flattened, elliptical structure with a discernible bulge that appears bright and concentrated towards the center. The overall color is dominated by redder hues, particularly within the central bulge, suggesting an older stellar population. Fainter, bluer colors are visible along the edges of what appears to be a faint disk component, possibly indicative of some ongoing star formation. While there is no distinct spiral structure, a slight irregularity or disturbance may be present, although further investigation is required to confirm whether this galaxy is undergoing any minor merging activity. The object appears to be relatively smooth and lacks prominent features associated with active galactic nuclei or major starburst regions.
