The galaxy appears to be an elliptical type, displaying a generally smooth, featureless morphology. Its overall shape is close to round, with a slight deviation towards an elongated form. The central region exhibits a higher luminosity, suggesting a concentrated stellar population or a possible active galactic nucleus. The galaxy's color profile trends towards the redder end of the spectrum, indicating a population of older stars and a relatively low rate of current star formation. No significant tidal disturbances or signs of recent mergers are readily apparent, suggesting a relatively isolated and quiescent evolutionary history. Faint, diffuse outer regions are visible, extending beyond the brighter core, implying a substantial galactic halo.
