The galaxy presents as a spiral type, with a notable central bulge exhibiting a yellowish hue, indicative of an older stellar population. Two less prominent spiral arms emanate from this central region. The arms display a bluer color, suggesting the presence of more recent star formation. There appears to be evidence of tidal disruption or interaction. There is a lopsided morphology that may indicate a previous merger event or ongoing gravitational interaction. The light profile suggests a relatively high Sersic index, consistent with a centrally concentrated structure.
