The galaxy presents a somewhat elongated, disk-like morphology. There is a central, bright region, likely a bulge, exhibiting a yellowish-white hue indicative of an older stellar population. Surrounding this central region, the disk displays a bluer tint, suggesting the presence of younger, hotter stars and possibly ongoing star formation. The disk appears relatively smooth, but with subtle irregularities that could indicate spiral arm structures or minor disturbances. Overall, the galaxy appears to be an intermediate spiral type, potentially undergoing some level of interaction or internal activity, with an estimated diameter of 6 kpc. The light distribution is fairly concentrated with an apparent visual magnitude of 18.44 in the g band.
