The galaxy appears as a single, relatively smooth object with a concentrated central bulge. There is a subtle elongation suggesting it might be elliptical in shape, but it doesn't appear highly flattened. The galaxy has a yellowish-orange hue, indicating a population dominated by older stars. There is no discernible dust lane or spiral structure visible. The object lacks any obvious signs of active star formation, supporting the conclusion that it's primarily composed of an older stellar population. There are no indications of tidal features or ongoing merger activity. It appears to be a relatively undisturbed system.
