The galaxy presents as a moderately luminous, elongated object. It exhibits a disk-like structure, with the major axis of the disk significantly longer than the minor axis. The color profile suggests a relatively evolved stellar population, with a dominant yellowish hue implying a prevalence of older stars. There appears to be a subtle dust lane or obscuration present, though the resolution limits definitive confirmation. There is some indication of a slight asymmetry in the distribution of light, which could imply some minor interaction. Star formation appears suppressed within the galaxy, corresponding with the high fraction of old stars. The estimated size appears to be consistent with a normal sized disk galaxy.
