The galaxy appears as an elongated, cigar-shaped system, viewed at a significant angle relative to its equatorial plane. It exhibits a relatively smooth morphology, with a bright central bulge that gradually fades into the outer regions. The central bulge presents a yellowish-white color, suggestive of an older stellar population. Fainter bluish hues are present in the surrounding disk, indicating the presence of younger, hotter stars, likely within spiral arm structures that are not clearly resolved. There is evidence of dust lanes within the disk, which contribute to the mottled appearance of the outer regions. The lack of significant morphological disturbances suggests the galaxy has not recently undergone a major merger event. Overall, the galaxy seems to be an intermediate mass system with a low rate of star formation and a significant fraction of old stars.
