The galaxy presents an elliptical morphology, appearing largely smooth and featureless. It exhibits a concentrated central bulge that is bright, with the luminosity decreasing gradually outward. The overall shape is somewhat elongated, transitioning from more rounded to a slightly cigar-shaped appearance. Evidence of disturbance, possibly from a minor merger event, appears present in the outer regions. The color gradient shows a subtle bluer hue concentrated towards the center, potentially indicative of a younger stellar population or ongoing star formation. The outer regions have a redder, fainter color, potentially indicating older, redder stars. No distinct spiral arms are apparent.
