The galaxy presents as a lenticular or possibly an elliptical galaxy, with a highly elongated, cigar-shaped morphology. It exhibits a relatively smooth, featureless appearance overall, lacking prominent spiral arms or distinct structures. The central region displays a concentrated, yellowish hue, likely indicating an older stellar population. Extending outwards from the core, the color transitions to a bluer tint, suggesting the presence of younger stars. There may be indications of some minor disturbances, but no prominent merging features are observed. The galaxy appears relatively isolated, with no immediate signs of gravitational interaction with other galaxies.
