The galaxy appears as an elliptical type, presenting a smooth, round morphology. Its color profile indicates a redder population, suggesting a prominence of older stars and a relatively low ongoing star formation rate.  There is a general lack of defined structures such as spiral arms or a prominent disk. The overall light distribution suggests a spheroidal shape, with a high degree of central concentration. Faint color variations are present but don't disrupt the overall homogeneity of the galaxy's appearance. There appears to be no signs of any major merger events or significant tidal disturbances.