The galaxy presents a generally elliptical morphology with a smooth, diffuse appearance, suggesting a relatively old stellar population. The central region exhibits a concentrated luminosity, indicative of a substantial galactic nucleus, possibly harboring a supermassive black hole. The color profile transitions from a reddish hue in the core, suggestive of older, redder stars and dust, to a bluer periphery, hinting at some recent star formation activity or a population of younger, bluer stars in the outer regions. There's little evidence of spiral arms or a well-defined disk structure. Minor asymmetry is present, possibly indicative of past or ongoing gravitational interactions, although no prominent tidal features are immediately apparent. Overall, the galaxy appears to be an evolved system undergoing relatively quiescent star formation.
