The galaxy presents as a primarily smooth object with a pronounced central bulge. Its shape appears to be elongated, with an axis ratio indicating a possible elliptical morphology. The color gradient suggests an older stellar population, concentrated towards the center. There is little evidence of distinct spiral arms or significant dust lanes. The overall structure is relatively undisturbed, with no obvious signs of major mergers or tidal interactions. Subtle features, such as minor disturbances, might be present, but are difficult to discern. The object has a modest size, typical of a dwarf galaxy, suggesting a low mass. The star formation activity appears to be subdued, consistent with a low star formation rate and a high specific star formation rate.
