The object presents as a spiral galaxy at an approximate distance calculated with a redshift of about 0.06. The galaxy shows both a smooth central bulge and some disk features. The central bulge region is relatively round and exhibits a smooth, diffused light, suggesting a population of older stars. The disk is visible, but indistinct and clumpy, with what may be spiral arm segments extending outwards from the core region, though these arms are not well-defined. Some minor disturbances and irregularities are visible in the disk, which could indicate tidal effects or minor interactions. The overall color profile implies a combination of stellar populations, with bluer regions possibly indicating ongoing star formation and redder regions suggesting older stellar populations. The light from the center seems to dominate over the disk.
