The galaxy presents as a relatively compact, elliptical-like system. It exhibits a smooth and largely featureless morphology, dominated by a central bulge. The color profile suggests a predominantly older stellar population, emitting strongly in the redder wavelengths. There is no evidence of significant disk structure or spiral arms. Faint tidal features cannot be ruled out due to the image resolution, although the system appears largely undisturbed, indicating it is not currently undergoing a major merger event. A subtle elongation is visible. Star formation appears to be largely suppressed, based on the red color and lack of blue, star-forming regions.
