The galaxy presents as a relatively smooth, centrally concentrated light distribution. Its overall form appears largely elliptical, exhibiting a high degree of roundness in its isophotes. There is a subtle color gradient, transitioning from a slightly bluer hue in the outer regions to a more yellowish color toward the core. This may indicate differing stellar populations with the core being more abundant in older, redder stars. There is no strong evidence of spiral arms or a distinct disk structure, nor signs of active galactic nuclei or other activity. The galaxy exhibits a slightly asymmetric brightness profile, possibly indicative of a minor interaction or past merger event, however, these signs are not major and there is nothing immediately indicating a merger. It's moderate luminosity suggests that the galaxy is reasonably massive.
