The galaxy presents a largely smooth, elliptical morphology. The light distribution appears centrally concentrated with a gradual decrease in surface brightness towards the outer regions. There is little evidence of distinct spiral arms or prominent dust lanes within the observed optical wavelengths. Color gradients suggest a slightly bluer core region, possibly indicating ongoing or recent star formation, although the overall appearance is dominated by older stellar populations exhibiting a redder hue. The galaxy displays no signs of significant tidal disturbances or interactions with other galaxies, suggesting it is relatively isolated and dynamically relaxed. The ellipticity is low, approaching a near circular shape. The overall structure points to a relatively evolved system that is likely undergoing only low levels of star formation, resulting in a dominant population of older, redder stars.
