The galaxy exhibits a somewhat elliptical morphology, appearing elongated rather than perfectly spherical. A central bulge is visible, characterized by a yellowish hue, suggesting a population of older stars. Surrounding the bulge is a fainter, more diffuse disk component. This disk presents a bluer color, indicative of ongoing star formation. There is a slight asymmetry or irregularity in the outer regions of the disk, which could be suggestive of tidal interactions or past minor mergers. Overall, the galaxy appears relatively smooth in texture, with no prominent spiral arms or large-scale disturbances readily apparent. The colors suggest a mix of stellar populations, with both older, redder stars concentrated in the bulge and younger, bluer stars distributed throughout the disk.
