The galaxy appears to be a relatively smooth, elliptical galaxy with a high degree of central concentration. Its morphology suggests a classification leaning towards an elliptical type due to its lack of discernible spiral arms or a prominent disk structure. The galaxy presents a generally round shape and appears largely undisturbed, with no obvious signs of major mergers or tidal interactions. There may be evidence of minor disturbances present. The color profile indicates an older stellar population, dominated by evolved stars, suggested by the redder hues observed towards the central bulge. Star formation appears low.
