The galaxy presents as a somewhat irregular structure, with a noticeable central concentration of light that suggests the presence of a bulge or core region. Extending from this core are faint, diffuse arms or features, which appear slightly disrupted and asymmetrical. There is evidence of potential tidal interactions, as indicated by the faint, extended features emanating from the main body of the galaxy. The overall color suggests a mixed stellar population, with both older, redder stars contributing to the bulge region and younger, bluer stars present in the fainter features. The galaxy displays characteristics of ongoing or recent star formation, though the rate appears relatively moderate. There might be a minor merger event occurring based on the structure.
