The galaxy presents as a relatively inclined disk galaxy, exhibiting a noticeable central bulge component that is more concentrated in luminosity. The bulge displays a yellowish-red hue, potentially indicating an older stellar population and/or significant dust extinction in that region. The disk component is less luminous and shows a bluer color profile, suggestive of the presence of younger stars. The galaxy's shape is not perfectly circular, but elliptical, with a major axis longer than its minor axis, supporting the disk interpretation. There's no clear evidence of prominent spiral arms, although subtle variations in the blue-ish light distribution within the disk might imply the presence of faint or tightly wound spiral structure. The galaxy appears relatively undisturbed, showing no obvious signs of major tidal interactions or mergers, but there may be some signs of minor disturbances.