The galaxy presents a largely smooth, elliptical morphology. Its shape is moderately rounded. The central bulge exhibits a bright, concentrated luminosity, appearing a warm yellow hue, suggesting an older stellar population. The surrounding disk is less defined, exhibiting a bluer color, which may indicate the presence of younger stars and some ongoing star formation, though at a low rate. There appears to be no significant dust lane or spiral arm structure visible in the image. There is no evidence of any major or minor mergers disrupting its form. Overall, the galaxy shows characteristics of a transitional object, potentially evolving from a spiral to an elliptical galaxy.
