The galaxy presents as a spiral type, exhibiting a prominent, though not overwhelmingly dominant, central bulge. A disk component is clearly visible, inclined slightly from a face-on orientation. Faint spiral arms emanate from the central region, displaying a somewhat tightly wound morphology. The overall color appears to be a mix of blue and yellow hues, suggestive of a stellar population that includes both younger, hotter stars in the spiral arms and older, cooler stars concentrated in the bulge. There may be some signs of minor disturbances or irregularities in the outer regions of the disk, potentially indicating interactions or past mergers. The galaxy appears relatively isolated, without a significantly close companion. The ellipticity of the galaxy is high, as its b/a value is close to 1, suggesting that it is nearly circular from our point of view.
