This galaxy exhibits a morphology characterized by a dominant smooth central component. The central region appears yellowish-white, suggesting an older stellar population. Extending from the central region, there is a fainter, bluish extension, which may indicate the presence of younger, hotter stars and regions of active star formation. The shape appears somewhat elongated or cigar-shaped, indicating a possible deviation from a purely elliptical form. There appears to be a minor disturbance or tidal feature present, with a possible interaction of the galaxy with a smaller object, or an internal event, leading to the observed asymmetry and extension. Overall, the galaxy is relatively compact in this image.
