The galaxy appears to be an elliptical galaxy, exhibiting a smooth and largely featureless morphology. It possesses a highly concentrated central bulge, characterized by a bright, yellowish hue. The galaxy's overall shape is nearly round with a slight elongation. There is no discernible evidence of spiral arms, dust lanes, or ongoing major merging activity. Faint, diffuse light extends outward from the central bulge, fading gradually into the background. The galaxy is characterized by an old stellar population, inferred from its color and morphology. There is no clear indication of active star formation regions. Overall, the galaxy appears to be a passively evolving system.
