The galaxy presents as a slightly elongated, elliptical structure with a bright, concentrated central bulge. The color profile exhibits a general shift towards redder hues in the central regions, suggesting an older stellar population. Fainter, bluer tints are observed in the outer regions, possibly indicating areas of more recent star formation. The galaxy shows no clear spiral arm structure. There is minimal visible dust obscuration across the galactic disk. Overall, the galaxy appears relatively undisturbed, lacking signs of significant tidal interactions or major merger events.
