The observed galaxy presents as a spiral type, with a prominent central bulge. Spiral arms are discernible, extending from the central region. The galaxy exhibits a moderate inclination relative to the observer's line of sight. A bar structure appears to be present, running through the central bulge. The galaxy does not appear to be undergoing a major merging event, although minor disturbances or interactions cannot be ruled out based on this image alone. The color gradient suggests the presence of both older stellar populations in the bulge and younger, bluer stars in the spiral arms.
