The galaxy presents as a relatively well-defined spiral structure, though the arms are not exceptionally prominent or tightly wound. There appears to be a notable central bulge that exhibits a yellowish hue. This suggests a potentially older stellar population dominating the core region. The spiral arms show bluer tones, which is indicative of younger stars and ongoing star formation. The galaxy's disk seems fairly smooth, lacking substantial clumpy structures or prominent HII regions that would suggest intense, localized star-forming activity. Overall, the galaxy appears to be a moderately active spiral galaxy with a mix of stellar populations. There might be a moderate level of star formation occurring within the disk.
