The galaxy presents as a generally smooth object with a concentrated central bulge. It appears elliptical or possibly lenticular in morphology, lacking any discernible spiral arm structure. The light distribution exhibits a gradual decline in intensity from the core outwards, suggesting a lack of prominent star-forming regions within the disk. The color profile indicates a higher concentration of older stellar populations, especially towards the center, which appears distinctly yellow or orange. There is very little evidence of dust lanes or any tidal features that would indicate recent interactions or mergers. Overall, the galaxy appears to be a relatively evolved system undergoing a period of quiescence or low star formation activity.
