The galaxy presents as a relatively smooth, elongated structure, likely a disk or elliptical galaxy viewed at an oblique angle. The central region exhibits a higher concentration of luminosity, suggesting a prominent galactic bulge or nucleus. The color profile appears slightly redder in the central bulge compared to the outer regions, which may indicate an older stellar population dominating the core and relatively younger stars in the outer regions. The galaxy lacks any obvious spiral arm structure or significant dust lanes visible in this image, hinting at either a smooth disk galaxy, an elliptical galaxy, or a spiral galaxy with tightly wound arms and minimal dust obscuration. There is no apparent major ongoing merging activity. The size suggests it is a fairly large galaxy. Faint extensions might be present, though they are not obvious in the data. Overall, the galaxy appears to be in a relatively quiescent state, with minimal star formation based on the lack of blue regions.
