The galaxy presents as a relatively smooth, centrally concentrated object with a primarily elliptical morphology. There is a lack of distinct spiral arm structures or prominent dust lanes discernible in the image. The light profile is relatively uniform, lacking any significantly bright knots or regions of intense star formation that would indicate a more irregular morphology.

The galaxy core appears bright and concentrated, with color suggesting an older stellar population, and with fainter light extending outwards in a mostly symmetrical halo. The galaxy appears slightly elongated along a major axis, and may have a very slight disk-like component with axis ratio near 1. The overall appearance is consistent with an elliptical galaxy, possibly of type E4.

There is no obvious evidence of tidal distortions or interaction with other galaxies, suggesting this is a relatively isolated system. Color variations are present and are very subtle, with the central core appearing slightly redder than the outer regions.
