The galaxy presents as a single, dominant spheroid with a smooth, relatively featureless morphology. The object exhibits a concentrated central region, suggestive of a substantial galactic nucleus. The overall color is a yellowish hue, indicating a stellar population dominated by older, redder stars. There is little evidence of spiral arms, dust lanes, or significant ongoing star formation activity. The galaxy appears well-defined and isolated, with no obvious signs of tidal interactions or ongoing merger events with neighboring galaxies.
