The galaxy appears to be a relatively luminous spiral galaxy, likely viewed at an intermediate angle, with a redshift of approximately 0.18. The central bulge is prominent and appears relatively smooth and concentrated, exhibiting a yellowish hue suggesting an older stellar population. The disk component is visible, though less clearly defined, showing a bluer color compared to the bulge, implying ongoing star formation. The spiral arms are not clearly resolved in the image, but there are hints of asymmetry or minor disturbances in the outer regions, possibly indicating a past minor merger or tidal interaction. Overall, the galaxy has a moderate size and mass, with an estimated active star formation rate.
