The galaxy presents as a spiral type, viewed at an oblique angle. A moderately sized bulge is visible, exhibiting a yellowish hue, possibly indicating an older stellar population. Faint spiral arms extend outward from the bulge, displaying subtle blue tones suggesting the presence of younger, hotter stars and regions of active star formation. The overall structure reveals some clumpy regions within the arms. The galaxy appears relatively isolated, showing no signs of major interaction or tidal disturbances with any neighboring galaxies.
