The galaxy presents as a relatively smooth, elongated structure. The overall color profile suggests a dominant population of older stars, exhibiting a redder hue, although the central region shows a hint of bluer light. The morphology appears to be cigar-shaped, exhibiting an elliptical structure with a high degree of elongation. There is no obvious evidence of spiral arms or significant dust lanes. The galaxy seems undisturbed, showing no apparent signs of recent major mergers or tidal interactions. Star formation rate seems to be low. The galaxy has a mass typical of the population of galaxies in the nearby universe.
