The galaxy presents as a central, luminous object. Its morphology appears largely smooth and elliptical, with a high degree of central concentration of light. I observe a subtle gradient in color, with the central region exhibiting a slightly yellower hue compared to the outer edges, which show a tendency towards redder tones. The lack of distinct spiral arms or prominent dust lanes suggests a classification leaning towards an elliptical or lenticular galaxy type. There is no obvious evidence of recent or ongoing major merger activity, although subtle irregularities in the outer regions could indicate past minor interactions or disturbances.
