The galaxy presents as an elliptical or lenticular morphology, exhibiting a smooth, concentrated light profile. The central bulge dominates the overall structure, with a somewhat rounded appearance. There are no prominent spiral arms or disk-like features easily discernible. The galaxy has an apparent color gradient, being bluer towards the core, transitioning to redder hues in the outer regions. This color shift could indicate a higher concentration of younger, hotter stars near the center, possibly due to recent star formation, while the outer regions may be dominated by older, cooler stellar populations. There is a slight indication of minor disturbance within the immediate vicinity of the galaxy, without significant signs of an ongoing major merger. The galaxy's estimated physical size is around 4 kiloparsecs.