The galaxy appears to be a relatively smooth, disk-like structure with a central bulge. The bulge exhibits a reddish hue, indicative of an older stellar population. The surrounding disk appears bluer, suggesting the presence of younger, hotter stars and ongoing star formation, though at a low rate. The galaxy shows no signs of major disturbances or mergers; it appears relatively isolated. It has a fairly circular shape, although there may be a slight deviation. There is no evidence of a strong spiral structure, it looks like a possible lenticular galaxy. The colors of the galaxy indicate it has moderate luminosity.
