The galaxy presents a generally smooth, elliptical morphology. It appears to have a concentrated central bulge exhibiting a yellowish hue, possibly indicative of an older stellar population. The outer regions gradually fade into a bluer halo, suggesting the presence of some younger, star-forming regions, although star formation appears minimal overall. The galaxy exhibits a moderately elongated shape and does not display any obvious signs of major disturbances or mergers, though subtle irregularities cannot be ruled out at this resolution. The overall structure suggests an evolved system, potentially transitioning towards a quiescent state.
