The galaxy exhibits an elongated, cigar-like morphology. Its light is relatively smooth and diffuse, lacking prominent spiral arms or significant substructure. The color profile suggests a population of older stars, with a reddish hue predominating, especially towards its core. The galaxy appears to be generally isolated, without any obvious signs of tidal interactions or ongoing mergers, though there is a slight disturbance, suggesting a very minor interaction. Overall, this galaxy appears to be a relatively quiescent system, possibly an elliptical or lenticular galaxy, at a moderate distance.
