The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated luminosity profile. Its shape is elongated, appearing cigar-shaped. The central region displays a yellowish-orange hue, potentially indicative of an older stellar population and dust presence. The outer regions of the galaxy fade gradually into the background sky, showing a less concentrated distribution of light. Faint blue-ish or green-ish regions appear, particularly around the edges, hinting at possible low-level star formation activity. There is no apparent evidence of strong tidal features or ongoing major mergers. However, a slight asymmetry in the outer regions cannot be excluded, suggesting a minor interaction or disturbance in the past.
