The galaxy presents a predominantly smooth morphology, suggesting an elliptical classification. The shape appears mostly round, with a slight deviation towards an intermediate form. There is no evidence of substantial merging activity or major disturbances to the overall structure. The light distribution suggests a concentrated central bulge, with luminosity decreasing gradually outwards. The galaxy exhibits a yellowish-red hue, indicative of an older stellar population and a low current star formation rate. There are no discernible spiral arms or prominent dust lanes visible in this image, further supporting the likelihood of an elliptical classification. The galaxy possesses an apparent size indicating substantial physical dimensions.
