The galaxy appears as an elongated, elliptical shape, suggesting a classification as either an elliptical galaxy (E) or a lenticular galaxy (S0). The light distribution is generally smooth and concentrated towards the center, indicating a higher stellar density in the core. There is little evidence of spiral arm structure or prominent dust lanes. The color gradient shows a yellowish-white hue throughout the galaxy, likely representative of an older stellar population. Its profile is more elongated than round. There are no apparent signs of active galactic nuclei activity or significant ongoing star formation regions discernable from this imagery. No major merging events or tidal disturbances are immediately evident. Overall, the galaxy presents as a relatively quiescent system, consistent with the visual impression of an evolved stellar population.
