The galaxy presents as a moderately bright, elliptical-like structure with a generally smooth appearance. It is elongated, tending toward an "in between" roundedness, rather than perfectly circular or highly cigar-shaped. The core appears to be intensely bright with a yellowish hue, suggesting a higher concentration of older stellar populations. Progressing outwards, the galaxy maintains a generally smooth texture with a subtle color gradient towards bluer tones, indicating pockets of younger stars or lower metallicity stellar populations. No prominent spiral arms or distinct features are visible, possibly due to the viewing angle and the galaxy's intrinsic morphological characteristics. There is no visual evidence of major mergers or strong tidal disturbances; however, a minor asymmetry or disturbance cannot be entirely ruled out based on this image alone.
