The galaxy presents as a somewhat elongated, lenticular-like structure, inclined at an angle to our line of sight. A bright, concentrated central bulge dominates the galaxy's luminosity. This bulge exhibits a yellowish-white color, suggesting an older stellar population. The surrounding disk appears significantly fainter and bluer in hue. The blue color is likely indicative of recent star formation. The disk's structure is not clearly defined; it appears relatively smooth with subtle hints of spiral arm features or dust lanes. At one end, there's a small region with enhanced redness, possibly indicative of localized dust concentration. There does not appear to be evidence of a strong interaction with other galaxies; the overall shape suggests a relatively undisturbed system.
