This galaxy appears to be a spiral galaxy viewed at a slight angle, possibly an intermediate spiral type. The central bulge exhibits a smooth, concentrated luminosity profile with a yellow-orange hue, indicating an older stellar population. Faint spiral arms extend outwards from the central region, displaying a mottled appearance. A hint of bluer light is present within these arms, suggesting the presence of younger, hotter stars and ongoing star formation, although the overall star formation rate is likely low. There is no clear evidence of a bar structure, and the spiral arms appear relatively tightly wound. No major mergers or significant tidal disturbances are visibly distorting the galaxy's overall morphology.
