The galaxy appears to be a relatively smooth, elongated elliptical galaxy. Its central region exhibits a bright, diffuse glow, indicating a concentrated population of stars. The overall color suggests a relatively old stellar population with low ongoing star formation. The galaxy is significantly elongated, approaching a cigar shape. There is no apparent sign of strong tidal disturbances or major merger events. There may be a hint of a minor asymmetry or disturbance, though it does not appear to be significant. The lack of visible spiral arm structures or prominent dust lanes is consistent with a classification as an elliptical galaxy with minimal recent star formation.
