This galaxy presents as a generally smooth object with a slightly elongated, cigar-like morphology. A central, concentrated bulge exhibits a yellowish-orange hue, suggesting a population of older stars and a relative lack of ongoing star formation in that region. Moving outwards from the core, there is a gradual transition to a fainter, bluer halo, hinting at the presence of a more dispersed distribution of younger, hotter stars. There is a subtle suggestion of a disk-like structure embedded within the halo, though this is not well-defined. The galaxy does not appear to be undergoing any major merger activity, though there may be minor disturbances in the outer regions, indicated by slight asymmetries in the light distribution. Overall, this galaxy likely resides in a mature state, potentially undergoing a period of quiescence in its star formation activity.