The galaxy presents as an elliptical morphology, with a high degree of central concentration.  The light profile appears smooth and largely featureless, lacking prominent spiral arms or a distinct disk structure. The color is generally redder, indicative of an older stellar population and/or significant dust extinction.  There is no obvious evidence of tidal tails or major disturbances suggesting recent major merger activity. Subtle disturbances or interactions might be present, but not readily discernible given the image resolution and the galaxy's apparent smoothness. The galaxy is approximately round in shape.
