This galaxy appears to be a spiral galaxy, viewed at a high inclination. It has a bright, concentrated central bulge, indicative of a significant stellar population. The disk is visible, though its structure is somewhat indistinct. The galaxy exhibits a generally smooth texture, although there is a suggestion of some disturbance or faint arm structures. There is a subtle color gradient present, with the central bulge appearing more yellow/white, potentially indicating an older stellar population, while the outer disk shows a slightly bluer hue, possibly suggesting ongoing or recent star formation activity. There is no obvious evidence of a major ongoing merger, though the galaxy's overall appearance suggests a possibility of some minor interaction or past gravitational disturbance.
