This galaxy appears to be a disk galaxy viewed at an oblique angle. The central region exhibits a bright, concentrated luminosity profile, suggesting a possible bulge component. The disk itself shows some evidence of internal structure, although image resolution limits detailed analysis. There are hints of spiral arm features. The galaxy's color is generally consistent with an older stellar population, though some bluer regions are present, possibly indicating areas of ongoing star formation. There appears to be some disturbance to the shape of the galaxy, potentially caused by a merger or interaction. The galaxy presents a hazy appearance, possibly due to dust obscuration or low-level tidal features.
