The galaxy presents as a relatively smooth, oblong-shaped structure. There is a brighter, slightly irregular central region, suggesting a higher concentration of stellar material and/or active galactic nuclei. This central region is distinctly bluer in color, possibly indicative of ongoing star formation. The overall color gradient shifts from a bluer core to a redder halo. The outer regions of the galaxy appear more diffuse and extended, gradually fading into the background. There is some evidence of possible minor disturbances in the galaxy's morphology, although the general structure appears to be fairly regular. It is difficult to determine with certainty from this image whether it is a pure elliptical or if it has a disk component viewed edge-on.
