The observed galaxy presents a somewhat elliptical morphology. A central bulge appears prominent and bright, exhibiting a concentrated luminosity gradient, with redder hues toward the center. The overall color suggests a population dominated by older stars. The presence of a disk may be indicated by the flattened shape, although clear spiral arm structure is not apparent. A faint, somewhat diffuse halo is visible, extending outward from the central region, exhibiting a bluer color profile relative to the bulge. Faint tidal disturbances extend from the central bulge in opposite directions, potentially suggestive of minor gravitational interactions. These features may warrant further investigation to determine the cause of these apparent disturbances. The galaxy's morphology is predominantly smooth; some minor irregularities exist, but these are not dominant structural features.
