The galaxy presents a generally smooth, elliptical morphology. The central bulge exhibits a bright, concentrated luminosity profile, suggesting a dense stellar population. The overall color is predominantly reddish-yellow, indicative of an older stellar population with relatively low ongoing star formation. There is very little evidence of spiral arm structure. A slight distortion or faint tidal feature may be present in the outer halo, hinting at a possible minor interaction or past merger event. The galaxy is roughly 8 kpc in diameter.