The galaxy presents as an elliptical morphology, appearing generally smooth in texture without prominent spiral arm structures or dust lanes. The light distribution is concentrated towards the center, with a gradual decline in luminosity as distance from the core increases. The galaxy's overall shape appears somewhat elongated. There is a lack of defined features, such as star-forming regions, that are visible. The color profile indicates a mature stellar population, with the galaxy appearing to be redder. There is no evidence of a recent or ongoing major merger event. Some small interactions cannot be ruled out with this picture, but the overall galaxy shape suggests that the galaxy has reached a stable equilibrium.
