The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The isophotes appear fairly regular, indicating a relaxed, dynamically evolved system. The color profile suggests a relatively old stellar population, with a slightly redder hue in the central regions transitioning to bluer colors in the outer halo. There is no strong evidence of spiral arm structure or a prominent disk component. Subtle indications of possible past minor interactions exist, potentially detectable as faint tidal features or asymmetries in the outer halo, although more detailed imaging would be required to confirm. The overall form is largely undisturbed, suggesting any interactions were either minor or occurred in the distant past. The estimated size is a few kiloparsecs in radius. The rate of star formation appears to be quite low.
