The galaxy presents as an elliptical morphology, exhibiting a generally smooth, centralized light distribution. The central region appears bright and concentrated, transitioning gradually to a fainter halo or envelope. There is a subtle color gradient visible, shifting towards redder hues in the core and somewhat bluer tints in the outer regions. No obvious spiral arms or distinct dust lanes are apparent, supporting the classification of an elliptical system. Minor irregularities in the outer regions suggest possible tidal interactions or minor disturbances in the galaxy's recent history.
