The galaxy presents as a relatively smooth, elongated structure. The light distribution suggests a central bulge, with a noticeable concentration of light, and an extended, fainter disk. There is no strong indication of well-defined spiral arms. The disk appears somewhat disturbed, with subtle asymmetries in its light distribution, and a hint of possible tidal features or minor interactions. The color appears to be somewhat redder in the bulge, consistent with an older stellar population, while the disk shows a bluer tint suggesting some ongoing star formation, although it may be at a low level. Overall, this galaxy seems to be an intermediate type, possibly an early spiral or a lenticular, with some signs of minor disturbances in its morphology.
