The galaxy presents a distinctly elongated, cigar-shaped morphology. Its light profile appears smooth, lacking any prominent spiral arms or well-defined disk structure. The central region exhibits a concentrated luminosity, suggesting a significant bulge component. The overall color index indicates a generally older stellar population, with a yellowish-red hue dominant throughout the galaxy. There are no obvious signs of recent or ongoing major mergers, although a slight asymmetry in the outer regions suggests the possibility of minor gravitational interactions. The object appears relatively isolated in the observed field.
