The galaxy exhibits a generally smooth morphology, with a high degree of central concentration. The light profile suggests an elliptical shape, appearing mostly round with a hint of elongation. There is a dominant central bulge exhibiting a yellowish hue, potentially indicative of an older stellar population. The galaxy is relatively isolated with minimal signs of tidal disturbance or interaction with other galaxies. The absence of well-defined spiral arms or prominent dust lanes further supports a classification towards the elliptical end of the Hubble sequence. There may be some faint blue light in the outer regions, potentially indicating areas of low-level star formation, though the smoothness of the overall profile suggests that any such star formation is not occurring at a high rate. The galaxy's color and smooth morphology suggest that this is a quite massive galaxy with the presence of older stars.
