The object presents as a relatively smooth, concentrated light distribution. The galaxy displays an overall elliptical morphology, though there is some subtle irregularity suggesting possible interactions or recent mergers. The central region is brighter and more densely packed than the outer regions. The galaxy exhibits a yellowish hue, indicative of an older stellar population with a low rate of active star formation. There is a possible tidal tail feature extending from one side, which is suggestive of a prior or ongoing gravitational interaction.
