The galaxy presents as a concentrated, elliptical morphology, with a high degree of central light concentration. The core is a bright, unresolved region exhibiting a yellowish hue, suggesting an older stellar population. The isophotes appear generally smooth and regular, lacking prominent spiral arm structures or significant dust lanes. There is a slight extension of the light distribution along one axis suggesting a mild deviation from perfect ellipticity. Faint, diffuse light extends outward from the central bulge, gradually fading into the background. A minor feature appears as a localized, slightly brighter region extending away from the main galaxy body along it's major axis suggesting a potential tidal interaction or ongoing accretion event. Overall the galaxy appears undisturbed.
