The galaxy appears to be an intermediate spiral type, showing characteristics of both elliptical and spiral galaxies. The central bulge is prominent and exhibits a smooth, yellowish-white color, suggesting an older stellar population. Fainter spiral arms extend outward from the bulge, appearing somewhat fragmented and less defined. The arms are bluer in color compared to the bulge, hinting at ongoing star formation. The galaxy does not seem to be perfectly symmetrical; a slight tidal distortion or minor interaction may be influencing its shape on one side. There is some indication of dust lanes within the spiral arms, though not very pronounced. The galaxy has a moderate redshift. The overall morphology suggests a galaxy that is possibly undergoing a minor merger or interaction with another galaxy, indicated by asymmetries, or may be a post-merger galaxy.