The galaxy presents a largely smooth, elliptical morphology. It appears moderately concentrated, with a slightly elongated shape that is in between round and cigar-shaped. There is no evident spiral structure, and the galaxy appears largely undisturbed. Its color index indicates a redder population of stars, suggesting an older stellar population with a reduced star formation rate. This is in agreement with the smooth morphology. There's a very slight suggestion of minor tidal disturbance, potentially indicating a past interaction or a very small merger. The galaxy is a dominant feature, and does not appear to be involved in any major ongoing merging events.
