The galaxy exhibits a disturbed morphology, suggestive of an ongoing or recent interaction. A prominent, bright central bulge is visible. Spiral arm structure appears present, exhibiting a relatively open winding. One side of the galaxy appears to have a more disturbed or elongated arm feature, with high star formation rates. This asymmetry, coupled with the overall irregular shape, supports the hypothesis of a gravitational interaction. The central bulge exhibits a yellowish-white coloration, potentially indicative of an older stellar population, while the spiral arm regions show bluer colors, suggesting younger, hotter stars associated with active star formation. Dust lanes may be present within the spiral arms, contributing to the observed color variations. The estimated physical size suggests a moderate disk galaxy.
