The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellowish-red hue, potentially indicative of an older stellar population and/or significant dust obscuration. A broader, less intense greenish halo surrounds the core, possibly tracing a distribution of cooler gas. The galaxy shows some evidence of minor disturbance in its outer regions. There may be weak evidence of a lopsidedness. The galaxy's morphology suggests it is likely in a relatively quiescent state, not undergoing any major merger events. There is very little evidence of actively forming stars.
