The galaxy presents a spiral morphology with a prominent central bulge. The bulge exhibits a yellowish hue, suggesting a population of older stars. Spiral arms are visible, though somewhat tightly wound, emanating from the bulge region. These arms appear slightly blue, likely due to the presence of younger, hotter stars and ongoing star formation. One arm is clearly defined and the other two are very short and difficult to see in detail. Dust lanes are present, appearing as dark regions within the spiral arms. There is no evidence of a strong bar structure. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, though there is some subtle distortion in the outer regions, hinting at possible minor interactions or internal dynamics. The galaxy appears relatively isolated in this image, which may suggest a small group environment.
