The galaxy presents as an elliptical morphology, exhibiting a generally smooth, featureless light distribution. The central region displays a concentrated, yellowish hue, suggesting an older stellar population. This core fades outward into a slightly bluer, more diffuse halo. The galaxy's overall shape is neither perfectly spherical nor highly elongated, leaning towards a more moderately elliptical form. No prominent spiral arms, dust lanes, or tidal features are discernible, indicating a lack of significant recent or ongoing merger activity. The absence of clearly defined structures supports a classification favoring a relatively quiescent, evolved system. Based on the observed color gradient and smooth profile, star formation appears to be relatively low.
