The galaxy presents as a central bulge surrounded by a fainter disk. The bulge exhibits a smooth, concentrated light profile, indicative of an older stellar population. The disk appears more complex, with hints of possible spiral arm structure. The arms are not well-defined, but there are areas with bluer tones suggesting regions of ongoing star formation, contrasted with areas of more yellow and red hues. Additionally, there are irregular features suggestive of a recent or ongoing interaction, particularly a possible tidal tail or extended emission to the lower center side. The morphology implies a system that may be undergoing transformation due to internal processes or external influences such as a minor or major merger event. Overall it appears to be a large and active galaxy.
