The galaxy presents as a relatively compact and smooth structure. Its morphology leans towards elliptical, with an intermediate degree of roundness but not perfectly spherical. There is a discernible lack of prominent spiral arms or a distinct disk-like feature. Instead, the light appears to be diffusely distributed across the galaxy's body, with a notable absence of strong, localized star-forming regions. Subtle hints of disturbance may be present, but the overall structure does not suggest a recent major merger. The color profile indicates a population dominated by older stars, with a fainter presence of younger blue stars. The galaxy shows a redder overall color compared to typical spiral galaxies.
