The galaxy presents an elliptical morphology, exhibiting a cigar-like shape in its overall structure. The light distribution appears relatively smooth across the galaxy's body, suggesting an older stellar population. The galaxy core shows a bright, concentrated region of light. Fainter extended emissions can be seen from the body, fading toward the edges of the structure. There is little evidence of spiral arm structures or significant dust lanes. No tidal tails or morphological indications of any ongoing major merging events can be clearly identified, but a small amount of local disturbance can not be ruled out based on morphology. Overall, the galaxy appears to be a relatively massive system, with moderate star formation.
