The galaxy presents as an elliptical morphology, exhibiting a high degree of central concentration. Its overall light distribution appears smooth, lacking any clear spiral arm structures or distinct features indicative of active star formation regions. The color profile leans towards the red end of the spectrum, suggesting an older stellar population dominated by evolved stars. The galaxy's shape is largely circular, showing a lack of significant elongation or tidal distortions. There is no evidence of ongoing or recent merger activity, as the system appears largely undisturbed with no visible tidal tails or asymmetries. Overall, the galaxy exhibits characteristics consistent with a mature elliptical galaxy with a relatively low star formation rate and a predominantly old stellar population.
