The galaxy presents an overall elliptical morphology, appearing predominantly smooth in texture. A pronounced central bulge is visible, displaying a yellowish-orange hue, suggestive of an older stellar population. Moving outwards from the core, the light appears to gradually fade into the background, with no distinct spiral arms or well-defined structures immediately apparent. A slight elongation is observable, classifying it somewhere between round and cigar-shaped. There is no obvious sign of interaction with other galaxies. The galaxy appears relatively isolated within its surrounding space, and there are no noticeable tidal tails or other distortions that might indicate a recent merger event.
