The galaxy appears to be an elliptical type, exhibiting a smooth, largely featureless morphology. The light is concentrated toward the center, indicating a prominent bulge. The color profile displays a gradient, transitioning from a redder hue near the core to slightly bluer tones in the outer regions. The galaxy presents an elongated shape, more cigar-like than circular. There's no obvious sign of spiral arms or significant dust lanes. Minor irregularities or disturbances can be observed, possibly hinting at a past interaction or minor merger event, however the system is mostly relaxed. The overall color suggests an older stellar population dominating the galaxy's composition, although some ongoing star formation cannot be ruled out based on the subtle bluer tones.
