The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely rounded in shape. There is no obvious spiral arm structure or bar visible in the image. The light profile appears to gradually decrease in intensity from the core outwards, lacking any sharp edges or distinct features.

The galaxy's color gradient transitions from a bluer hue in the core to slightly redder tones in the outer regions. This suggests a possible difference in stellar populations, with the core potentially hosting a larger fraction of younger, hotter stars compared to the outskirts. There are no signs of significant ongoing mergers or major disturbances affecting its morphology. The overall appearance is consistent with a galaxy that has largely exhausted its gas supply and is dominated by an older stellar population, though a measurable level of recent or ongoing star formation is not ruled out.
