The galaxy presents as a slightly elongated, intermediate-stage spiral, possibly between Sa and Sb types. A bright, concentrated central bulge is visible. The arms are moderately wound and somewhat indistinct. There is a general smoothness to the morphology, suggesting that it's dominated by older stellar populations. The galaxy exhibits an overall yellowish-red hue, indicative of a population dominated by older stars, potentially with a low star formation rate. There are hints of dust lanes and possibly some regions of ongoing, low-level star formation within the disk, evidenced by some bluer areas within the spiral arms. Overall, the galaxy does not appear to be undergoing any major mergers or significant tidal disturbances.
