The galaxy presents as a relatively smooth, elliptical-like structure, exhibiting a concentrated central bulge. The light distribution appears centrally condensed, fading gradually towards the outer regions. There's a subtle color gradient, transitioning from a more yellowish-orange hue in the core to a slightly redder tone in the outer regions. Given the morphology and color profile, the galaxy likely contains an older stellar population, with ongoing, but relatively low levels of star formation. There is some indication of mild tidal distortion, suggesting potential past or ongoing gravitational interactions with other galaxies.
