The galaxy appears to be an elliptical galaxy. It exhibits a relatively smooth, featureless morphology with a high degree of central concentration. The galaxy has an elongated shape, suggesting it is not perfectly spherical. The color profile exhibits a radial gradient, with a reddish hue dominating the central region, which likely signifies an older stellar population. Moving outwards, the galaxy transitions to a bluer hue, indicating the presence of a younger stellar population. The galaxy appears relatively isolated, with no visible signs of major mergers or significant tidal disturbances. However, the presence of a very slight irregularity suggests a possible minor interaction or disturbance in its past. Based on the color profile, the galaxy appears to be a red and dead galaxy, with most star formation occurring in the outer edges.
