The galaxy presents a generally smooth and elliptical morphology, appearing somewhat rounded in shape. There is a bright, concentrated central bulge exhibiting a yellowish-orange hue, suggestive of an older stellar population. The light gradually diminishes with increasing radius from the core. Hints of bluer colors are visible in the outer regions of the galaxy, possibly indicating some degree of recent or ongoing star formation there. No prominent spiral arm structures or signs of a recent major merger event are readily apparent. The overall impression is of a relatively quiescent galaxy, although subtle disturbances cannot be ruled out based on this image alone. The galaxy appears to be reasonably massive, given its apparent luminosity and size.
