This galaxy exhibits a generally smooth morphology with a slight elongation, appearing somewhat cigar-shaped. The light is concentrated in a central bulge, which presents with a yellow-orange hue, suggesting a population of older stars. There's a gradual decrease in luminosity moving outward from the bulge, creating a diffuse halo. No distinct spiral arms or prominent dust lanes are discernible. A very small amount of blue light is visible in the outer regions of the galaxy, pointing towards the possibility of minor pockets of ongoing star formation. Overall, the galaxy appears undisturbed, without any obvious signs of recent or ongoing mergers.
