The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. Its color profile suggests an older stellar population, exhibiting a yellowish hue that dominates the overall appearance. There is no distinct spiral arm structure or prominent dust lane visible; the light distribution appears relatively uniform and symmetric around the core. The galaxy's shape approximates a near-circular ellipse. No obvious signs of tidal disturbances or ongoing major mergers are detected. Subtle color variations exist, with the central region appearing more intensely yellow compared to the slightly redder outer regions. This may indicate a radial gradient in stellar population age and/or metallicity. The galaxy's apparent size is small, suggestive of its large distance, which would explain why the presence of minimal star formation activity is hard to see.
