The galaxy presents as a roughly elliptical structure with a concentrated, bright central bulge. The light distribution appears smooth, suggesting a relatively well-mixed stellar population. The galaxy appears somewhat lenticular as the bulge is surrounded by what could be a faint, diffuse disk. The absence of prominent spiral arms or significant dust lanes indicates a lack of ongoing, large-scale star formation. The overall color profile suggests a dominance of older, redder stars. There is no obvious evidence of tidal tails or strong morphological distortions, indicating that the galaxy has not recently undergone a major merger. Minor disturbances cannot be ruled out.
