The galaxy appears to be an elliptical or lenticular type, exhibiting a smooth, concentrated central bulge. There is an apparent absence of distinct spiral arms or prominent dust lanes. The galaxy's light profile suggests a relatively uniform stellar population, with a gradual decline in brightness from the core outwards. The color indices indicate a population of older stars dominating, with a generally redder hue.

The shape suggests a slightly elongated spheroid, indicating some degree of flattening. There is no visible evidence of recent mergers or major disturbances in its structure, although subtle asymmetries or tidal features cannot be ruled out. The overall morphology is consistent with a galaxy that has undergone significant evolutionary processing.
