The galaxy presents as a central, somewhat amorphous, slightly elongated object with a diffuse halo. The central region exhibits a bright, concentrated luminosity, possibly indicative of an active galactic nucleus or a dense stellar population. The color profile transitions from a bluish-white core to a reddish-yellow outer region, potentially suggesting a mix of young, hot stars in the center and older, cooler stars in the periphery. There appear to be some disturbed features, possibly indicative of tidal interactions or recent merger activity, suggesting that the galaxy is not completely relaxed. The low central-to-total light ratio points to a relatively young stellar population. The overall structure suggests a transitionary stage, possibly evolving from a late-type spiral to an elliptical galaxy, with considerable star formation ongoing, particularly in the core region. The galaxy appears relatively compact.
