The galaxy presents as a moderately compact, elliptical or lenticular type. It exhibits a smooth, largely featureless morphology, with a high degree of central concentration. The color profile suggests a population dominated by older stars, appearing yellowish-orange in this rendering. No distinct spiral arms or bar structures are discernible. The galaxy exhibits a slight asymmetry, possibly due to a minor interaction or internal dust lane, however, this requires further investigation. There is no evidence of active star formation regions within the visible extent of the galaxy.
