The galaxy presents as a luminous, elongated structure. Its central region exhibits a concentrated glow, transitioning outward to a more diffuse halo. There appears to be a slight asymmetry to the overall form, suggesting a potential tidal interaction or recent merger event, though no prominent tidal tails are visible. The color profile indicates an aging stellar population, dominated by redder wavelengths, with only hints of bluer components, possibly indicating ongoing but subdued star formation. The observed smoothness of the galaxy's light distribution is suggestive of an elliptical morphology.
