This galaxy appears as a moderately bright object with a smooth overall morphology. It exhibits a slightly elongated, disk-like shape rather than a perfect sphere. There is no strong evidence of major disturbances or ongoing mergers within the galaxy's structure, although there might be some minor irregularities. The color profile indicates the presence of both older stellar populations, which contribute to the redder hue, and some younger, bluer stars suggesting ongoing or recent star formation, likely at a relatively low rate. The galaxy is relatively compact.
