The galaxy presents as a centrally concentrated object, likely an elliptical galaxy given its smooth, featureless appearance and overall roundness. There is no obvious spiral arm structure or evidence of a prominent disk. The central region exhibits a bright, yellowish hue which fades to a redder, less intense color in the outer parts, suggesting a population of older stars with diminished recent star formation. Some very minor disturbances can be seen upon further inspection, but these do not appear to constitute a major merger event. The galaxy is slightly elongated in shape, but not strongly so. No obvious tidal tails or other signs of significant gravitational interaction are seen.
