The galaxy presents as a spiral type, observed at an angle oblique to its primary plane. It displays a prominent central bulge, which constitutes a substantial fraction of the galaxy's overall luminosity. This bulge exhibits a smooth, yellowish color, indicative of an older stellar population. Fainter spiral arms are discernible emanating from the central region and seem to extend outwards. The arms lack sharp definition and the contrast appears low. Overall, the galaxy appears relatively smooth in texture, but not perfectly elliptical. There is no indication of any active galactic nucleus or significant starburst activity from this observation.
