The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a spheroid-dominated morphology, possibly an elliptical galaxy or a lenticular galaxy seen nearly edge-on. The core exhibits a bright, somewhat compact, yellow-white appearance, indicating a likely older stellar population. A faint, diffuse blueish halo surrounds the central bulge, potentially indicating the presence of some younger, bluer stars or ongoing, albeit low-level, star formation. The overall shape is elongated, appearing cigar-shaped, with no obvious spiral arm structure or significant dust lanes visible. There are no signs of any major ongoing mergers or significant tidal disturbances. The galaxy exhibits a red shift value suggesting it is a fairly distant object.
