The galaxy presents as a spiral galaxy, viewed at an angle that is neither face-on nor edge-on. The central bulge is prominent and exhibits a yellowish-white hue, potentially indicating a population of older stars. The spiral arms are well-defined, displaying a bluish tint characteristic of ongoing star formation activity, and a two-armed morphology appears to dominate the spiral structure. These arms are moderately wound. There is no obvious bar feature. The galaxy appears to be in a relatively isolated state, showing no significant signs of major tidal disruption or ongoing merger activity.
