The galaxy presents as a relatively compact object. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars or potentially an active galactic nucleus. The surrounding region displays a fainter, more diffuse glow, which may indicate a stellar halo or a disk component, though definitive features are not readily apparent. The light distribution appears somewhat irregular, potentially hinting at past or ongoing interactions. There may be minor disturbances as well, although the resolution makes any determination tentative. The overall color suggests a mix of stellar populations, with both younger, bluer stars and older, redder stars contributing to the observed light. 
