The galaxy appears to be an elliptical galaxy, characterized by a smooth, diffuse light distribution without prominent spiral arms or a well-defined disk. Its shape is noticeably elongated, with the major axis extending roughly horizontally in the image. The color profile suggests a population of older stars, with the central region displaying a yellow-orange hue indicative of lower star formation rates and a higher proportion of red giant stars. The galaxy exhibits a high degree of central concentration, with luminosity gradually decreasing from the core to the outer edges. There is no apparent dust lane or other signs of significant gas or dust content. The overall morphology suggests a relatively evolved galaxy, likely formed through the merger of smaller galaxies or through the slow accretion of matter over cosmic time.