The galaxy presents as a somewhat disturbed spiral or lenticular galaxy, though potentially transitioning between the two. A central bulge is quite apparent, exhibiting a yellowish-white hue, possibly indicative of an older stellar population. A faint disk component is also discernible. The disk structure exhibits a slight blueness, particularly in some regions, possibly indicating ongoing star formation. There appear to be tidal features, with the disk showing evidence of minor disturbances. Some faint spiral arm segments may exist, though they appear somewhat disrupted, giving the galaxy an irregular appearance. Overall, the galaxy displays a morphology hinting at a possible past or ongoing merger event, evidenced by the distorted disk and potential tidal features.
