The galaxy presents an elliptical morphology, appearing largely smooth in texture with a discernible central bulge. Its color profile leans towards the blue end of the spectrum suggesting a relatively younger stellar population or ongoing star formation, although the absence of clearly resolved spiral arms or HII regions implies that such activity may be subdued or confined. The galaxy appears to be of moderate luminosity, occupying an intermediate size on the image plane. There is a slight elongation of the galactic structure indicating a possible deviation from a perfectly spherical form. The overall structure suggests an evolved system, potentially transitioning towards a more quiescent phase of galactic evolution. There are no immediately apparent signs of major mergers or significant tidal disturbances within the observed morphology, though more subtle interactions cannot be ruled out.