The galaxy presents as a moderately sized, likely lenticular or early-type spiral system, with a prominent central bulge. The bulge exhibits a yellowish-orange hue, suggesting an older stellar population. What appears to be a disk or arm structure is visible, but it is relatively faint. There is very little evidence of ongoing star formation within this area. It displays a somewhat uniform light profile, without significant irregularities or bright knots indicative of active star-forming regions. The overall morphology suggests a galaxy undergoing minimal interaction with other galaxies, and no distinct tidal features or signs of a major merger. However, there may be minor disturbances present.
