The galaxy appears as a single, somewhat diffuse object with a concentrated central bulge region. The overall shape is elliptical, exhibiting a high degree of roundness. There is no visible spiral structure or distinct disk component. The light profile appears smooth and centrally concentrated, with a gradual decrease in intensity outwards from the bulge. The color is generally yellowish-orange, indicating an older stellar population. No significant dust lanes or active star-forming regions are readily apparent in this image. There is no indication of any major disturbances or ongoing merger activity. A secondary, smaller, and slightly dimmer component is visible near the primary galaxy, possibly a smaller galaxy or a bright star cluster. The light from this component is similar in color.
