This galaxy appears to be an elliptical type, exhibiting a smooth, featureless morphology with a concentrated central bulge. The light distribution is highly centralized, showing a radial decrease in intensity from the core outwards. The galaxy appears to be relatively round in shape and shows no signs of significant tidal disturbances or interactions with other galaxies. Its color suggests a population dominated by older stars, emitting primarily in the redder wavelengths, with relatively low current star formation activity. There is no evidence of a prominent disk structure.
