The galaxy presents as a relatively bright, elongated structure. A central bulge is visible, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Surrounding the bulge is a disk component. This disk shows a slightly bluer color than the bulge, which suggests the presence of younger, hotter stars and ongoing star formation, although the color is more muted. The disk appears relatively smooth with some indications of spiral arm structure, though poorly defined. The galaxy is observed at an inclined angle, giving it an elliptical appearance. There is no clear evidence of strong tidal features or major mergers, although the overall morphology appears slightly disturbed.
