The galaxy presents as a centrally concentrated, ellipsoidal structure, exhibiting a relatively smooth morphology. The galaxy's core displays a bright, yellowish hue, indicative of an older stellar population. This color suggests a diminished rate of current star formation within the nuclear region.

Surrounding the core, the galaxy's light gradually fades into an extended halo. This outer region exhibits a bluer color, suggesting the presence of some younger, hotter stars, although they are much less prominent than the stars in the core. There is no obvious spiral structure and no pronounced tidal features or distortions are apparent, indicating that it has likely not undergone any major mergers recently. The smooth overall appearance and lack of significant substructure suggests a relatively quiescent evolutionary state.

Overall, this galaxy appears to be a moderately massive, relatively evolved system, with a dominant population of older stars and a subdued amount of on-going star formation.
