The galaxy presents a dominant, centrally concentrated spheroid morphology. The light profile appears relatively smooth, indicating a lack of prominent spiral arms or strong dust lanes. However, upon closer inspection, a subtle disk-like component can be observed. The elongation suggests it is cigar shaped. The galaxy exhibits a color gradient, appearing bluer in the central region and redder towards the outer edges. This suggests ongoing star formation is primarily located in the nucleus or inner disk, with an older stellar population dominating the outer regions. The absence of clear tidal features or morphological distortions implies it has not experienced a recent major merger event, though some minor disturbances may be present.
