The galaxy presents a somewhat elongated, cigar-shaped morphology. Its light profile appears relatively smooth, lacking prominent spiral arms or distinct features. The color gradient suggests a concentration of older stellar populations toward the center, indicated by the yellowish hue, possibly implying a significant bulge component. The outer regions exhibit a bluer color, hinting at the presence of younger, hotter stars and ongoing star formation, though this activity appears moderate. There's no obvious evidence of a major merger or significant tidal disturbances. The galaxy’s structure is largely undisturbed, suggesting a stable evolutionary history. It seems to be a relatively massive galaxy, judging by its overall luminosity and size.
