This galaxy exhibits a generally smooth morphology. The central region appears significantly brighter, indicative of a concentrated stellar population, possibly a bulge. Moving outward from the center, the light profile gradually diminishes. There's evidence of a flattened disk component extending beyond the bright central region. The overall shape appears to be somewhere between rounded and elongated. Faint, irregular structures are present in the outer regions, possibly indicative of minor disturbances. No major merger events are immediately apparent. The color profile indicates a population of relatively old stars dominating the light output, with minimal indication of recent, ongoing star formation. The object appears relatively isolated, with no obvious signs of tidal interactions.
