The galaxy exhibits a prominent bulge, appearing as a concentrated, bright region at the center, likely composed of older stellar populations. This galaxy appears to be a spiral galaxy, as it does exhibit some features that could be spiral arms. These arms are not distinct and tightly wound, being of a more flocculent nature, displaying patches of star formation. The galaxy is oriented at an angle to our line of sight, appearing elliptical. There is evidence of a bar structure bisecting the bulge, though it is not especially dominant, indicating that this bar is either faint or partially obscured. The disk of the galaxy appears relatively smooth, with no major disturbances or merging activity visible. The overall color of the galaxy suggests a mix of stellar populations, with the bulge being more yellow/orange, indicative of older, redder stars, and the disk showing slightly bluer regions.
