The galaxy presents as a well-defined, flattened spheroid. Its overall color profile is dominated by yellowish hues in the central region, suggestive of an older stellar population. This core blends smoothly into outer regions with subtly bluer tones, potentially indicating more recent star formation at the galactic edges. The galaxy exhibits a moderate degree of ellipticity. There is no visible evidence of strong spiral arm structures or significant tidal disturbances. The galaxy appears relatively isolated, with no obvious close companions or merger events in progress. Overall, it seems to be a relatively undisturbed system.
