The galaxy presents as a largely featureless elliptical morphology. The light distribution appears smooth and centrally concentrated, lacking prominent spiral arms or a well-defined bar structure. The object's shape is generally round. There is no evidence of tidal tails or other significant distortions suggestive of a recent major merger. The galaxy exhibits a moderate redshift, indicating a substantial distance. The color profile suggests a population of older stars, with a relatively low rate of ongoing star formation. Subtle indications of minor disturbances might be present, such as a faint asymmetry in the outer regions, but these are not pronounced.
