The galaxy appears to be elliptical, exhibiting a smooth, centrally concentrated morphology. The galaxy's light profile indicates a lack of distinct spiral arms or a prominent disk structure. The color gradient suggests an older stellar population, with a yellowish hue dominating the central regions, transitioning to slightly redder tones toward the periphery. There is no apparent dust lane or significant evidence of ongoing star formation visible in this image. The galaxy is relatively isolated with little to no tidal distortion from gravitational interaction with any nearby galaxies.
