The galaxy presents as a slightly disturbed, intermediate-type spiral galaxy with a redshift of approximately 0.21. Its overall morphology appears to be dominated by a relatively smooth, bright central bulge. The surrounding disk component exhibits a more diffuse structure. There are faint hints of spiral arms. The color profile shows a shift towards redder hues. This suggests a presence of older stellar populations and perhaps some degree of dust obscuration, although the overall star-formation rate is relatively modest. There are hints of a possible minor disturbance, although nothing definitive. The galaxy's shape is somewhere between round and elongated.
