The galaxy presents as a relatively small, lenticular structure, with a smooth, diffuse appearance. Its morphology suggests a classification leaning toward an elliptical galaxy, though with some subtle elongation. There is a slight concentration of luminosity towards the center, hinting at a possible galactic nucleus, albeit not particularly active. The color profile is predominantly consistent, with a slight reddening compared to younger galaxies. Faint spiral arms are not readily discernible, pointing towards a later stage of galactic evolution, potentially with diminished star formation rates. The absence of prominent dust lanes further supports this assessment, suggesting a well-mixed stellar population. Overall, it appears to be a quiescent galaxy, likely composed of older stars. There is a slight indication of possible tidal disturbance nearby in the form of a small plume. It is difficult to tell if the plume is directly related to the primary object. Further analysis would be beneficial.
