The galaxy presents as a relatively smooth, elliptical morphology with a high degree of central concentration. It is characterized by a dominant spheroid component, with a discernible elongation along its major axis. The color profile suggests an older stellar population, with a yellowish hue concentrated toward the central bulge. Faint blueish edges may imply subtle star formation occuring on the outer edges of the galaxy. No prominent dust lanes or spiral arm structures are visible. No evidence of strong tidal interactions or major mergers are apparent; there might be some minor gravitational disturbance. Overall, it presents as a galaxy with no active star formation within its core.
