The galaxy appears as a single, fairly smooth object with a slightly elliptical shape. A central bulge is visible, exhibiting a yellowish-orange hue, suggesting an older stellar population. The surrounding disc, while less prominent, shows a bluer color, possibly indicative of ongoing star formation. There is no strong evidence of spiral arms or a distinct bar structure. No significant tidal disturbances or signs of a major merger are readily apparent, although there is the possibility of a minor disturbance based on asymmetry. The galaxy's overall structure suggests a relatively evolved system, potentially an early-type spiral or a lenticular galaxy.
