The galaxy presents a largely smooth morphology, appearing elliptical in shape with a high degree of central concentration. There is little evidence of spiral arms or a well-defined disk structure. The galaxy exhibits a color gradient, with a yellowish-white core, transitioning to a redder hue in the outer regions. This suggests a stellar population dominated by older, redder stars in the outer regions. The overall luminosity profile appears smooth, further supporting the interpretation as an elliptical galaxy with minimal dust obscuration or active star formation. There is no clear indication of any major mergers or significant tidal disturbances affecting its morphology. Subtle, localized regions of bluer light are visible near the center of the galaxy, implying the presence of younger, hotter stars, albeit at a lower rate compared to typical star-forming galaxies.
