The galaxy presents as a slightly inclined spiral with a prominent central bulge. The bulge region exhibits a yellowish-white hue, suggesting an older stellar population and/or significant dust obscuration. Faint spiral arms extend outwards. The arms appear somewhat patchy and fragmented, with subtle blue tints suggestive of ongoing star formation. The galaxy has a relatively smooth overall appearance with little evidence of major tidal disturbances or recent merger activity. The disk of the galaxy is tilted relative to our line of sight, giving it an elliptical appearance.
