The galaxy appears to be an elongated, disk-like structure, viewed at a significant angle. Its overall color profile suggests an older stellar population, appearing redder in color. The central bulge region is prominent and appears smooth, with the light becoming less concentrated as it moves away from the center towards the edges of the disk. There is some evidence of a slight asymmetry in the outer regions of the disk. While no distinct spiral arm structures are visible, this could be due to the angle of observation, limitations of image resolution, or the intrinsic morphology of the galaxy itself. There is no obvious central star formation. The shape of the galaxy is highly elongated. There is a possibility of some minor gravitational disturbance or interaction, though the image is not clear enough to confirm any ongoing merging activity. Overall, the galaxy appears to be a relatively quiescent disk galaxy, with a dominant bulge and evidence of an aging stellar population.
