The object presents as a spiral galaxy with a prominent central bulge. The bulge exhibits a yellowish-white hue, possibly indicative of an older stellar population. Two distinct spiral arms emanate from the central bulge, displaying a relatively defined structure. The arms exhibit a moderate winding pattern, appearing neither tightly wound nor loosely extended. Faint bluish regions are distributed throughout the spiral arms, potentially signifying areas of active star formation. A bar-like structure appears to bisect the central bulge. The overall morphology suggests that the galaxy is undergoing normal galactic evolution, and does not appear to be in the throes of a major merger or significant tidal disruption.
