The galaxy presents as a moderately inclined spiral with a relatively smooth disk structure. The central bulge appears diffuse, lacking a sharp, well-defined nucleus. There's faint evidence of spiral arm structure, with hints of disruption or tidal features, although it's relatively minor. The galaxy's overall color suggests a population of older stars, but it does also seem to have at least some star formation present. The shape is elongated, deviating from a perfect circle. There is no strong evidence of an ongoing major merger, but there is the possibility of minor interactions or internal disturbances.
