The galaxy presents an overall elliptical morphology, appearing somewhat rounded in shape. The central region exhibits a concentrated, bright core, suggesting a substantial stellar population. There is evidence of a more extended halo or disk surrounding this core, though the overall structure appears dominated by a spheroidal component rather than a well-defined spiral structure.

Slight color variations are noticeable, with a subtle shift towards redder hues in some areas. This may imply variations in stellar populations and/or dust content within the galaxy. There is evidence of a possible merger or tidal disturbance, as suggested by the asymmetrical shape and extensions of the galactic arms. Some irregular features within the galaxy suggest that the object may have undergone a recent interaction or is currently undergoing one. The mass of the galaxy is expected to be very large, as it can be seen across a large distance. Star formation is present, but at a relatively subdued rate.
