The galaxy presents as a moderately luminous, elongated structure. It exhibits a smooth overall morphology, with no prominent spiral arms or bar structures readily apparent. The light distribution suggests a centrally concentrated bulge, fading gradually outwards. The galaxy's color appears relatively uniform, with a slight tendency towards redder hues which may indicate an older stellar population and reduced ongoing star formation within the disk. Its shape indicates that it is likely an elliptical galaxy, and may possibly be undergoing some minor interaction with another galaxy.
