The galaxy presents as a somewhat elliptical structure with a relatively smooth, concentrated central bulge. The light distribution appears brightest and most condensed at the core, gradually fading outwards. The bulge region exhibits a subtle bluish hue, suggestive of the presence of a population of younger, hotter stars or ongoing star formation. Fainter extensions or arm-like features are barely discernible extending from the central region. These extensions show slightly more variation in color, hinting at some patchiness possibly caused by dust lanes or regions of enhanced star formation. The overall shape suggests a disk galaxy viewed at an angle, though the absence of well-defined spiral arms means it could be a lenticular galaxy.
