The galaxy presents a generally smooth, elliptical morphology. It appears largely featureless, lacking prominent spiral arms or bar structures. Its color profile is dominated by redder hues, with a bright, yellowish-white core fading into a reddish-brown halo. There is no obvious dust lane obscuring the nucleus. The light is centrally concentrated, suggesting an older stellar population and limited ongoing star formation. There is no evidence of a recent major merger or significant tidal disruption. A slight asymmetry is observed, though it is not significant. The galaxy appears to be a relatively evolved system.
