This galaxy exhibits a prominent spiral structure. The arms are well-defined and appear somewhat patchy, indicative of ongoing star formation. They emanate from a central bulge, which appears moderately sized. There is evidence of a bar-like structure in the central region, though it is not particularly strong. The galaxy presents a slightly inclined disk. The color profile suggests a mix of stellar populations, with bluer regions likely corresponding to younger stars in the spiral arms and a redder central bulge potentially containing older stars. The overall morphology shows no signs of significant tidal disruption or major mergers. The galaxy displays a relatively smooth texture, but with noticeable clumpy features within its spiral arms, hinting at active star-forming regions.
