The galaxy presents as an elliptical morphology, though it is not perfectly circular. It appears to be elongated, tending toward a cigar shape. Its light distribution is mostly smooth, with a brighter central region that fades gradually towards the edges. There isn't a clear indication of spiral arm structures or significant dust lanes; the structure is largely amorphous. The color gradient suggests a population of older stars, as indicated by a reddish hue that becomes more prominent at the edges. There is no obvious evidence of a recent major merger or significant tidal disturbance affecting the overall galactic form.
