The galaxy presents as a moderately inclined disk system. A bright, concentrated central bulge is prominent, exhibiting a yellowish hue suggestive of an older stellar population. The disk appears relatively smooth with a notable absence of clearly defined spiral arm structures. The outer regions of the disk exhibit a fainter, diffuse luminosity. The overall shape is elongated, indicating a significant inclination with respect to the observer's line of sight. The aspect ratio of the disk suggests a flattened morphology. No significant dust lanes or prominent star-forming regions are readily discernible. The lack of distinct features might indicate a relatively quiescent galaxy with a low star formation rate.
