The galaxy presents as a lenticular or possibly a spiral galaxy viewed nearly edge-on. Its morphology suggests a relatively smooth structure with a subtle disk component, although the near edge-on view makes it challenging to discern detailed features. The galaxy's color profile indicates a population of older stars, with a relatively low rate of ongoing star formation. The elongated shape, classified as cigar-shaped, could be a result of its intrinsic structure or a projection effect due to its orientation relative to our line of sight. There is no prominent central bulge that can be seen, nor signs of any major ongoing mergers or significant tidal disturbances that could have influenced its present shape. The galaxy's smooth appearance suggests that it is currently in a relatively quiescent state.
