The galaxy presents a smooth, elliptical morphology. It exhibits a concentrated central bulge that gradually fades into the surrounding halo. The galaxy appears to be mostly featureless, lacking prominent spiral arms or distinct dust lanes. The light distribution suggests an older stellar population, indicated by the overall yellowish hue. The elongated shape is moderately extended. There is no visible evidence of ongoing major mergers or significant tidal disturbances, although there is a slight asymmetry that suggests a potential minor interaction.
