The galaxy presents as a relatively smooth, elliptical structure with a dominant central bulge. The light distribution is concentrated towards the center, indicating an older stellar population. There is no obvious disk structure, spiral arms, or bar feature. The galaxy displays a generally round morphology. The color appears to be slightly redder in the central region, suggesting a higher concentration of evolved stars, possibly due to a lack of recent star formation activity there. There is no evidence of significant tidal disturbances, merging activity, or other signs of interaction with neighboring galaxies. The overall impression is of an isolated, passively evolving system with a considerable mass. The galaxy appears quite compact in size.
