This galaxy presents as a moderately bright, relatively smooth object with an elliptical morphology. The central region exhibits a high degree of light concentration, appearing almost stellar in its intensity. There are faint extensions or possible tidal features present, though these are not well-defined and may be the result of minor disturbances. The overall color profile suggests a moderate amount of ongoing star formation. The galaxy exhibits a slight asymmetry, possibly indicative of a past or ongoing interaction. There is no clear evidence of a prominent disk or spiral structure. The relative smoothness and rounded shape are consistent with a classification towards the elliptical end of the Hubble sequence.
