The galaxy presents as a single, concentrated object with a smooth morphology. There is no visible evidence of spiral arms or a distinct disk structure. The light profile appears generally round with an elliptical shape, lacking any significant distortions or tidal features that would suggest a recent major merger.

The galaxy's color is concentrated in the redder portion of the spectrum, implying a stellar population dominated by older, redder stars and/or significant dust extinction, which is consistent with a relatively low rate of star formation. There is no evidence of bright, blue star-forming regions typically found in actively star-forming galaxies. There are no significant disturbances nearby, although they could be very small and not obvious.
