The galaxy appears to be an elliptical type, exhibiting a relatively smooth morphology with a cigar-shaped appearance. There is a hint of a disturbance within the galaxy, possibly due to a past or ongoing minor interaction or merger event with a smaller object, evidenced by the asymmetrical distribution of its light. The central region shows a brighter, more concentrated luminosity, suggesting an older stellar population. The galaxy has a slightly redshifted color profile, indicating a substantial distance. Though difficult to fully resolve, there are signs of active or recent star formation regions.
