The galaxy presents as an elliptical or lenticular structure, exhibiting a high degree of smoothness in its light distribution. There is minimal evidence of spiral arms or a distinct disk component. The central region shows a concentrated, bright core, likely a galactic bulge or active galactic nucleus, which appears to be slightly off center. The light intensity diminishes gradually from the core outward, lacking any sharp edges or distinct features. The color profile indicates a yellow to reddish hue, possibly suggesting an older stellar population with lower levels of ongoing star formation. There is a faint hint of blue on the outer edges of the galaxy, which could be regions of limited star formation. The overall morphology appears undisturbed, without significant tidal tails or signs of recent mergers.
