The galaxy exhibits an overall elongated, cigar-shaped morphology. A bright, concentrated central nucleus is visible. Surrounding the nucleus is a fainter, more diffuse halo. Hints of a disk-like structure are observed, potentially indicating the presence of spiral arms, although these features are not sharply defined and the galaxy's overall shape appears more elliptical. Color gradients are present, with the central region exhibiting a blue-ish hue, suggesting a younger stellar population and potential ongoing star formation. The galaxy exhibits a moderate redshift, indicating it is at an appreciable cosmological distance. There might be a very faint merging event happening, but it cannot be seen clearly. 
