The galaxy appears as a moderately bright, somewhat rounded structure. It exhibits a concentrated central bulge that dominates the overall light profile. The color of the galaxy is generally yellowish, suggesting a population of older stars, though it has some bluer areas that indicate younger star formations, The light distribution appears relatively smooth, with a hint of a disk-like feature but without well-defined spiral arms, indicating it is likely a spiral galaxy. There is no obvious evidence of a major ongoing merger or tidal interaction.
