The galaxy appears as a moderately luminous object with an apparent elongation. The central region exhibits a bright, concentrated core, suggestive of a significant stellar population density. A diffuse, more extended halo surrounds the core, displaying a gradual decrease in luminosity with increasing distance from the center. The color profile shows a gradient, with the central regions exhibiting a yellowish hue, possibly indicating an older stellar population, while the outer regions show a slight bluish tint, which might indicate the presence of younger stars or ongoing star formation. There is no obvious spiral structure or distinct morphological features within the disk. Overall, the galaxy presents a smooth, somewhat featureless appearance, possibly indicating an elliptical or lenticular morphology. There appears to be no obvious evidence of recent major merger events or significant tidal disturbances.
