The galaxy presents as a relatively bright, moderately sized object, approximately elliptical in shape. The central bulge is prominent and appears largely featureless, exhibiting a smooth, concentrated light distribution. The brightness decreases gradually from the center outwards, indicating a diffuse halo structure. The major axis is slightly elongated. There is a faint hint of a possible disk-like structure, however, the image resolution is low, and its presence cannot be definitively confirmed. There is no clear evidence of active star formation regions within the visible spectrum, suggesting either an older stellar population or significant dust obscuration. There is no obvious indication of spiral arms or a bar. Overall, this galaxy appears to be a fairly typical elliptical galaxy. There appears to be very little or no ongoing star formation. No merger is visible in this image.
