The galaxy presents as a centrally concentrated object with a smooth, diffuse morphology. There's a general elliptical shape, exhibiting a gradual decrease in luminosity from the core outwards. While there are no obvious spiral arm structures or prominent dust lanes visible, some subtle variations in color suggest potential underlying features. The galaxy appears to be relatively undisturbed, without any major signs of ongoing mergers or tidal interactions. The color profile suggests a mature stellar population, implying low specific star formation rate. The majority of the light appears to be emitted from stars.
