The galaxy presents as a centrally concentrated, luminous object with a relatively smooth morphology. The color appears to be generally yellow-red, indicating a stellar population that is dominated by older, redder stars and/or significant dust extinction. The object exhibits a generally elliptical shape, with a high degree of roundness. There is no apparent evidence of spiral arms, distinct disk structures, or ongoing major merger activity in the visible light. Subtle color gradients are possibly present, with the central region being somewhat more yellow than the outer regions, perhaps signifying differing stellar populations. The lack of strong blue light suggests a low current rate of star formation.
