The galaxy presents as a somewhat elliptical, disk-like structure seen at an oblique angle. It exhibits a centrally concentrated bulge, with a smooth, diffuse halo extending outwards. The color profile suggests a higher concentration of older stellar populations within the bulge, displaying a yellowish hue, while the outer disk appears slightly bluer, potentially indicating more recent star formation. There's a subtle indication of possible disturbances or tidal features, evidenced by slight asymmetries in the outer regions of the disk, though no definitive major merger or disruption is immediately apparent. The galaxy shows an intermediate roundness. Overall, it appears as a relatively isolated system, without any strong, obvious signs of intense ongoing interaction with nearby galaxies.
