The galaxy presents as a single, largely featureless object. Its morphology is primarily smooth, with no prominent spiral arms or bar structures evident. The overall shape is roughly elliptical, appearing fairly round but tending towards a cigar shape. The core is bright and concentrated, suggesting a significant stellar population. The color gradient transitions from a yellowish core to slightly redder hues in the outer regions, which may indicate an older stellar population towards the galaxy's periphery. There is no visual evidence of ongoing major mergers or significant tidal disturbances; however, some slight irregularities might hint at minor interactions.
