The galaxy appears to be an elliptical galaxy, potentially of type E4-E5. It exhibits a smooth, concentrated central bulge which decreases in luminosity radially outwards. The galaxy's overall shape is moderately elongated, resembling a cigar shape. There are no obvious spiral arms or other features typically associated with disk galaxies visible. The light distribution is largely homogenous throughout the galaxy, which exhibits an overall blue-white hue, suggesting the presence of a moderate population of young, hot stars, though these stars may be primarily located in the core. There is no evidence of any significant ongoing merging activity or major disturbances within the galaxy's structure. The galaxy appears isolated and relatively undisturbed.
