The galaxy presents a largely smooth, elliptical morphology, appearing nearly circular in projection. The central region exhibits a high surface brightness, indicative of a concentrated stellar population. A subtle color gradient is observed, with the core appearing slightly more yellow-orange, suggesting an older stellar population and/or dust obscuration compared to the fainter, bluer outskirts. No distinct spiral arm structures or prominent dust lanes are discernible. The galaxy appears relatively isolated, although there is a slight asymmetry, suggesting a possible minor interaction.