The galaxy presents as a moderately inclined disk, appearing somewhat elongated in shape. Its central region exhibits a bright, concentrated bulge that diminishes gradually towards the edges of the disk. The color profile suggests a higher concentration of older stellar populations in the bulge, shifting to slightly bluer hues in the outer disk, possibly indicating regions of more recent star formation. There are some minor disturbances present in the disk, but they are not significant enough to classify this as a merging galaxy. It displays an intermediate roundness, appearing as a distorted ellipse with some hints of spiral structure embedded.