The galaxy presents a largely smooth, elliptical morphology. The central region exhibits a concentrated luminosity, suggesting a significant stellar population. The light profile appears generally featureless, with no distinct spiral arms or prominent dust lanes visible at this resolution. The galaxy appears moderately rounded, with a slight deviation from perfect circularity, indicating a possible ellipsoidal shape. There is no obvious evidence of ongoing major merger activity or significant tidal disturbances. There is an absence of distinctly blue regions. Overall, the galaxy appears to be a relatively evolved system, likely with a low star formation rate.
