The galaxy appears as a fairly luminous, centrally concentrated object with a generally smooth morphology. It exhibits a largely elliptical shape with a high degree of roundness. The color profile indicates an older stellar population, appearing more yellow in the central regions and transitioning to a slightly redder hue in the outer regions. There is no clear evidence of spiral arms or a prominent disk structure. Additionally, there are no obvious signs of ongoing major merging events or significant tidal disturbances. The galaxy's light profile decreases smoothly from its core, lacking any strong indications of star formation or patchy dust lanes. Overall, it presents as a relatively evolved galaxy with characteristics of an elliptical or lenticular type.
