The galaxy appears to be a disc galaxy with a relatively bright, concentrated core. The central region is luminous, exhibiting a cyan hue. The light distribution suggests the presence of ionized gas, potentially indicating active star formation in the core. The outer regions of the disk exhibit a mottled texture, with hints of spiral structure. The galaxy appears to be relatively undisturbed, without obvious signs of a major merger or tidal interactions. Some faint bluing is present in the outer disk, which may be indicative of some ongoing low level star formation in these regions. The galaxy is well defined, with only a few artifacts noted.