The galaxy presents as a relatively smooth, elongated structure. The central bulge exhibits a concentrated brightness, suggesting a high stellar density and potentially an older stellar population. The color of the central bulge appears to be more yellowish, consistent with older, cooler stars. The disk, while present, appears somewhat attenuated or tightly wound. The disk's color appears slightly bluer than the bulge, hinting at the presence of younger, hotter stars and ongoing star formation, although likely at a low rate. There is no immediately obvious evidence of strong spiral arm structure or significant tidal disturbances. The galaxy exhibits an overall elliptical or lenticular morphology. Any interactions with other galaxies are not readily apparent within the limitations of this observation.
