The galaxy presents a predominantly smooth morphology, with a notable lack of distinct spiral arm structures or prominent dust lanes. Its overall shape is elliptical to lenticular, appearing elongated rather than perfectly spherical. The central region exhibits a concentrated brightness, suggesting a bulge component with older stellar populations. Moving outward from the core, the galaxy's luminosity gradually decreases. The color profile indicates a yellow to reddish hue, consistent with a galaxy dominated by evolved stars and a low star formation rate. There is little evidence of ongoing mergers or significant tidal disturbances. It shows a low-level of disk activity with no clear signs of spirals.