The galaxy presents an elliptical morphology, with a noticeable flattening along its major axis. The core region exhibits a bright, concentrated luminosity profile, suggesting a high density of stars. A faint, diffuse halo surrounds the central region, gradually fading into the background. The overall color appears to be yellowish-white, indicative of an older stellar population, with subtle hints of bluer regions possibly indicating areas of recent or ongoing star formation, though these are minimal. No distinct spiral arm structure is visible. The galaxy appears relatively smooth, with no major disturbances or signs of mergers. The elongated shape suggests a significant inclination relative to the observer's line of sight.
