The galaxy presents as a moderately luminous object exhibiting a generally smooth morphology. Its shape is elongated, deviating from a perfectly circular form. It appears to be a relatively undisturbed system, lacking obvious signs of major mergers or significant tidal disruptions. There is subtle evidence of what might be a faint, extended disk, though the overall light distribution suggests a bulge-dominated structure. The galaxy's color is consistent with an older stellar population, indicating relatively low levels of on-going star formation. There is a hint of a central concentration of light, likely representing the galactic nucleus.
