This galaxy presents a relatively smooth, elliptical morphology. Its light profile is dominated by a central bulge that graduates in intensity outwards, with no obvious distinct features or spiral arm structures visible. The core appears yellowish and somewhat brighter, suggesting an older stellar population. The outer regions of the galaxy exhibit a gradual decline in surface brightness, with a subtle transition toward a slightly bluer color as distance increases from the center. This may indicate a younger stellar population in the outer regions compared to the central bulge. There is no indication of a strong merger event or tidal disturbances; the general form appears relaxed and largely undisturbed. Overall, the galaxy seems to be an evolved system.