The galaxy presents a generally smooth, elliptical morphology, with a high degree of central concentration. The light profile appears to be relatively uniform, lacking distinct spiral arms or bar structures. There is minimal evidence of significant dust lanes or patchy star formation regions within the galaxy's body. It exhibits a slightly oblate shape, showing some deviation from perfect circularity. No significant merger activity or tidal disturbances are readily apparent in this image. The color index suggests a relatively red population, potentially indicating an older stellar population and suppressed star formation. The object has an estimated effective radius, derived from its Petrosian radius, of approximately 7 kpc.
