This galaxy exhibits a predominantly smooth morphology, characterized by a concentrated central bulge. There is a disk component present, but it appears disturbed. The outer regions show faint, diffuse light, extending approximately 6-7 kiloparsecs from the core. Evidence of minor tidal interactions is discernible, possibly indicating past or ongoing merging activity. Star formation appears to be present but modest within the disk. The galaxy is likely a late-type spiral undergoing transformation.
