The galaxy appears to be a relatively smooth, elliptical-like structure. Its core is a prominent, bright orange hue, suggesting an older stellar population dominating this region. Moving outwards from the core, the galaxy transitions to a more diffuse, yellowish-white glow. This suggests the presence of a mix of stellar populations, possibly with some ongoing, albeit relatively low, star formation. The galaxy exhibits no apparent spiral arm structure or significant dust lanes. There are no major distortions or irregularities observed, indicating that the galaxy is likely not undergoing a major merger event. It has a somewhat rounded shape but seems to have an edge leaning towards cigar shaped. The surrounding region is relatively clear, with no obvious signs of tidal debris or nearby interacting galaxies. Overall, the galaxy presents as a well-defined, evolved system with a notable central concentration of older stars.
