The galaxy presents a moderately disturbed morphology, indicating possible interaction or merger activity. A prominent central bulge is observed, displaying a yellowish hue, suggestive of an older stellar population. Extending from the central bulge is a fainter disk component, exhibiting a bluer color profile, indicating areas of active star formation. Evidence suggests an ongoing or recent merger event with a distinct tidal tail extending away from the main galactic body, further emphasizing the disturbed nature. The overall structure appears to be elongated, deviating from a perfectly circular morphology.
