The galaxy presents as a spiral type, exhibiting well-defined spiral arms extending from a noticeable central bulge. The arms display a clumpy morphology indicative of active star formation regions, characterized by bluish hues. The central bulge appears yellowish and somewhat extended. A slight bar-like feature is suspected across the central region. No major signs of ongoing mergers or significant tidal disturbances are apparent, though minor irregularities in the outer arms cannot be discounted. The galaxy is not viewed edge-on, and its disk appears somewhat inclined to our line of sight.