The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light profile appears generally featureless with no visible spiral arms, bars, or dust lanes. The galaxy exhibits a color gradient, transitioning from a redder hue in the core to a bluer color in the outer regions. This color gradient suggests that the central bulge is dominated by an older stellar population, while the outskirts may host younger, bluer stars. There is no obvious evidence of recent or ongoing major merger activity or significant tidal disturbances. The galaxy appears to be a fairly isolated system.
