The galaxy appears to be an elliptical galaxy, characterized by a smooth, centrally concentrated light distribution. It is elongated in shape, displaying a cigar-like morphology. There is a dominant bulge component that appears yellowish, potentially indicating an older stellar population with lower rates of ongoing star formation. Faint, diffuse extensions are present surrounding the central region, suggesting a stellar halo. There is no clear evidence of spiral arms or a prominent disk structure. No significant signs of tidal disturbances or merging activity are discernible.
