The galaxy presents as a relatively faint, extended object with a flattened, disk-like morphology. The central region appears somewhat smooth in texture and exhibits a slight concentration of light, suggesting a possible bulge component, though it is not particularly pronounced. There are hints of fainter, less defined arm-like structures extending outwards from the central region. The overall color appears reddish, indicating a population of older stars, dust obscuration, or a significant redshift. There may be a small degree of tidal disturbance or asymmetry in the outermost regions, which could possibly be indicative of past or ongoing interaction with another galaxy, although it is not a merger.
