The galaxy presents a smooth, elongated morphology, appearing as a flattened spheroid rather than a distinct spiral or irregular structure. The central region exhibits a concentrated luminosity, suggesting a prominent galactic nucleus. The overall color profile indicates a relatively older stellar population, evidenced by the redder hue concentrated in the core, which likely dominates the galaxy's light output. Fainter, blue tinged light is seen in the outer halo, which suggests lower levels of star formation. There are no readily apparent signs of major mergers or tidal disturbances, although a faint asymmetry is observed on one side, possibly indicative of minor gravitational interactions or internal dynamics. The galaxy's structure implies a system dominated by older stars with limited ongoing star formation activity.
