The galaxy presents a generally smooth, elliptical morphology. The light distribution indicates a centrally concentrated luminosity profile, suggesting a prominent bulge component. The galaxy exhibits a yellow-white core, which may be indicative of an older stellar population. There is a very slight hint of bluer light extending outwards from the central region, possibly indicating some low-level ongoing star formation. No prominent spiral arm structures or dust lanes are apparent within the image resolution. The galaxy appears relatively isolated and does not obviously interact with any other galaxies. There may be some minor asymmetry in the outer regions, hinting at past or ongoing minor interactions. Overall, the galaxy appears as a typical elliptical galaxy with a possibly old and somewhat passively evolving stellar population.
