This galaxy exhibits a disk-like morphology with indications of disturbances. Approximately half of the galaxy appears smooth and centrally concentrated, while the remaining portion shows features suggestive of a disk structure. There is some evidence of ongoing interaction or merging activity, as indicated by possible tidal tails or asymmetries in the galaxy's outer regions. Star formation activity appears to be low throughout the galaxy, with little evidence of prominent HII regions or dust lanes. The galaxy displays a moderate redshift. Overall, this galaxy appears to be undergoing a relatively quiescent period, with morphological features suggesting a previous interaction or merger event.
