The galaxy presents as a mostly smooth, elliptical-like structure with a concentrated central bulge that graduates into a faint halo. There appears to be no strong evidence of spiral arm structure, but there is a slight flattening suggestive of a disk-like component. The color profile is dominated by yellowish hues in the central region, transitioning to reddish tones in the outer regions. This color gradient likely indicates an older stellar population in the central bulge and outskirts, consistent with a lower rate of recent star formation. There are subtle irregularities in the outer halo, but no readily apparent signs of ongoing major merger activity or significant tidal disturbances. The galaxy's morphology is mostly consistent with an evolved system, possibly an early-type spiral transitioning to a more lenticular form.
