The galaxy presents an overall elliptical morphology with a smooth, concentrated central bulge. The color profile appears redder towards the center, indicating a likely older stellar population. Fainter, bluer hues are observed in the outer regions, suggesting the presence of younger, star-forming regions, albeit weakly. The isophotes exhibit a slight elongation along a preferred axis, deviating from a perfectly circular shape, although no strong bar structure is apparent. There's no readily discernible spiral arm structure or any indications of recent major merger events. Minor disturbances cannot be ruled out due to the limited resolution. The galaxy appears relatively isolated, with no immediately obvious signs of tidal interactions with neighboring galaxies.
