The galaxy presents a largely smooth, elliptical morphology. It exhibits a bright, concentrated central bulge that appears approximately spherical. The light from this central region dominates the overall luminosity of the galaxy. A fainter, more diffuse halo surrounds the bulge, gradually fading into the background. The color profile shows a tendency toward redder hues, especially in the core, which may indicate an older stellar population. There is a lack of discernible spiral arm structure or dust lanes, furthering the assessment of an elliptical classification. The galaxy appears relatively undisturbed, showing no obvious signs of a recent major merger or tidal interactions. It has an estimated size of approximately 5 kiloparsecs.
