The galaxy presents as an elliptical-type system, with a smooth, symmetrical light distribution. The central region is dominated by a bright, concentrated core, indicative of an older stellar population. The galaxy's light profile gradually diminishes outwards from the core, showing a lack of distinct spiral arm structures or prominent dust lanes. There is a subtle color gradient, appearing slightly redder towards the center, which suggests a radial variation in stellar populations, possibly with older, redder stars concentrated in the nucleus. The overall morphology implies that this galaxy is relatively evolved, having undergone significant merging and star formation activity in the past, which has largely ceased in the present epoch. Faint, extended features may be present, potentially indicating tidal streams or remnants of past interactions, though these are not distinctly defined. The galaxy exhibits a moderate redshift, suggesting it resides at a significant cosmological distance.
